This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz
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 07 10.3333 2461231.8333 12.13 02:36:03.68 +32:37:34.9
147.17168 -25.27409 galactic Tri Second-epoch detections are separated by 0.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:03.68 +32:37:34.9 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.029 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:03.68 +32:37:34.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:03.68 +32:37:34.9: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 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!
TCP 2026 07 10.3333* 02 36 03.68 +32 37 34.9 12.1 U Tri 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,2461231.8333,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.90 02:33:46.91 +42:22:20.8
142.37875 -16.60189 galactic And Second-epoch detections are separated by 4.2" and 8.3 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 | 02:33:46.91 +42:22:20.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.276+/-0.028 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:46.91 +42:22:20.8: 12.76 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:46.91 +42:22:20.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 33 46.91 +42 22 20.8 11.9 U And 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,2461231.8333,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.06 02:35:03.83 +32:43:36.4
146.91436 -25.27419 galactic Tri Second-epoch detections are separated by 5.3" and 7.9 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 | 02:35:03.83 +32:43:36.4 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.028 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:03.83 +32:43:36.4: 13.13 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:03.83 +32:43:36.4: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 35 03.83 +32 43 36.4 12.1 U Tri 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,2461231.8333,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.13 02:36:39.20 +33:02:02.2
147.09997 -24.85294 galactic Tri Second-epoch detections are separated by 1.9" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:39.20 +33:02:02.2 (user input) | T | P | (position from user input) J-Ks=0.702+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:39.20 +33:02:02.2: 13.13 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:39.20 +33:02:02.2: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 36 39.20 +33 02 02.2 12.1 U Tri 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,2461231.8333,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.99 02:34:00.08 +42:34:00.3
142.33610 -16.40767 galactic And Second-epoch detections are separated by 6.3" and 8.4 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 | 02:34:00.08 +42:34:00.3 (user input) | T | P | (position from user input) J-Ks=0.242+/-0.029 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:00.08 +42:34:00.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:00.08 +42:34:00.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 07 10.3333* 02 34 00.08 +42 34 00.3 12.0 U And 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,2461231.8333,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.04 02:38:34.73 +34:14:21.3
146.91901 -23.59352 galactic Tri Second-epoch detections are separated by 2.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:38:34.73 +34:14:21.3 (user input) | T | P | (position from user input) J-Ks=0.587+/-0.026 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:38:34.73 +34:14:21.3: 13.09 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:38:34.73 +34:14:21.3: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 38 34.73 +34 14 21.3 12.0 U Tri 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,2461231.8333,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.88 02:33:46.78 +32:39:13.0
146.67874 -25.45592 galactic Tri Second-epoch detections are separated by 1.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4468+32.6420 | 02:33:46.78 +32:39:13.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.812+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:46.78 +32:39:13.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:46.78 +32:39:13.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 33 46.78 +32 39 13.0 11.9 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4468+32.6420,2461231.8333,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4468+32.6420 20260710.3333 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.00 02:35:52.71 +33:12:52.0
146.85277 -24.76048 galactic Tri Second-epoch detections are separated by 1.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:35:52.71 +33:12:52.0 (user input) | T | P | (position from user input) J-Ks=0.295+/-0.030 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:52.71 +33:12:52.0: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:52.71 +33:12:52.0: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 35 52.71 +33 12 52.0 12.0 U Tri 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,2461231.8333,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.00CV 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 07 10.3333 2461231.8333 12.05 02:40:48.85 +33:38:35.2
147.66145 -23.92301 galactic Tri Second-epoch detections are separated by 1.3" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J040.2035+33.6433 | 02:40:48.85 +33:38:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.986+/-0.028 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:40:48.85 +33:38:35.2: 13.08 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:40:48.85 +33:38:35.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 40 48.85 +33 38 35.2 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J040.2035+33.6433,2461231.8333,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J040.2035+33.6433 20260710.3333 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.12 02:30:37.29 +33:16:34.6
145.72476 -25.16816 galactic Tri Second-epoch detections are separated by 0.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6549+33.2762 | 02:30:37.29 +33:16:34.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.339+/-0.030 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:37.29 +33:16:34.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:37.29 +33:16:34.6: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 30 37.29 +33 16 34.6 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.6549+33.2762,2461231.8333,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.6549+33.2762 20260710.3333 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.05 02:35:16.33 +33:05:46.6
146.78260 -24.92177 galactic Tri Second-epoch detections are separated by 1.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8181+33.0960 | 02:35:16.33 +33:05:46.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.381+/-0.030 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:16.33 +33:05:46.6: 13.06 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:16.33 +33:05:46.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 07 10.3333* 02 35 16.33 +33 05 46.6 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.8181+33.0960,2461231.8333,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.8181+33.0960 20260710.3333 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.93 02:39:05.59 +33:54:14.3
147.18433 -23.84799 galactic Tri Second-epoch detections are separated by 0.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.7732+33.9036 | 02:39:05.59 +33:54:14.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.337+/-0.028 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:39:05.59 +33:54:14.3: 12.84 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:39:05.59 +33:54:14.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 39 05.59 +33 54 14.3 11.9 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.7732+33.9036,2461231.8333,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.7732+33.9036 20260710.3333 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.90 02:29:19.51 +32:42:27.0
145.70917 -25.79839 galactic Tri Second-epoch detections are separated by 1.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:29:19.51 +32:42:27.0 (user input) | T | P | (position from user input) J-Ks=0.645+/-0.026 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:19.51 +32:42:27.0: 12.83 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:19.51 +32:42:27.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 29 19.51 +32 42 27.0 11.9 U Tri 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,2461231.8333,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.98 02:42:07.47 +34:02:06.3
147.73483 -23.45061 galactic Tri Second-epoch detections are separated by 1.7" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 134723610725506816 | 02:42:07.35 +34:02:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:42:07.47 +34:02:06.3: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:42:07.47 +34:02:06.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 07 10.3333* 02 42 07.47 +34 02 06.3 12.0 U Tri 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 134723610725506816,2461231.8333,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134723610725506816 20260710.3333 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.93 02:31:02.51 +33:46:11.7
145.58828 -24.68232 galactic Tri Second-epoch detections are separated by 0.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:31:02.51 +33:46:11.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:02.51 +33:46:11.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:02.51 +33:46:11.7: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 31 02.51 +33 46 11.7 11.9 U Tri 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,2461231.8333,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.04 02:31:28.54 +33:26:50.6
145.82587 -24.93859 galactic Tri Second-epoch detections are separated by 1.9" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:31:28.54 +33:26:50.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.610+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:28.54 +33:26:50.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:28.54 +33:26:50.6: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 07 10.3333* 02 31 28.54 +33 26 50.6 12.0 U Tri 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,2461231.8333,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.99 02:31:47.79 +33:50:43.0
145.71098 -24.54886 galactic Tri Second-epoch detections are separated by 2.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9525+33.8488 | 02:31:47.79 +33:50:43.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.358+/-0.030 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:47.79 +33:50:43.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:47.79 +33:50:43.0: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 31 47.79 +33 50 43.0 12.0 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9525+33.8488,2461231.8333,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9525+33.8488 20260710.3333 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.98 02:30:37.88 +32:45:31.5
145.96359 -25.63858 galactic Tri Second-epoch detections are separated by 1.2" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:30:37.88 +32:45:31.5 (user input) | T | P | (position from user input) J-Ks=0.731+/-0.027 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:37.88 +32:45:31.5: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:37.88 +32:45:31.5: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 30 37.88 +32 45 31.5 12.0 U Tri 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,2461231.8333,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.81 02:29:14.64 +33:11:12.3
145.47484 -25.36793 galactic Tri Second-epoch detections are separated by 0.7" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:29:14.64 +33:11:12.3 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:14.64 +33:11:12.3: 12.83 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:14.64 +33:11:12.3: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 29 14.64 +33 11 12.3 11.8 U Tri 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,2461231.8333,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.06 02:33:12.12 +34:25:31.3
145.73597 -23.90036 galactic Tri Second-epoch detections are separated by 0.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:33:12.12 +34:25:31.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.419+/-0.029 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:12.12 +34:25:31.3: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:12.12 +34:25:31.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 33 12.12 +34 25 31.3 12.1 U Tri 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,2461231.8333,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.89 02:34:46.96 +32:50:45.9
146.79874 -25.19181 galactic Tri Second-epoch detections are separated by 1.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:34:46.96 +32:50:45.9 (user input) | T | P | (position from user input) J-Ks=1.082+/-0.086 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:46.96 +32:50:45.9: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:46.96 +32:50:45.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 34 46.96 +32 50 45.9 11.9 U Tri 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,2461231.8333,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.88 02:30:01.93 +32:56:09.1
145.75546 -25.52919 galactic Tri Second-epoch detections are separated by 0.5" and 8.8 pix
The object was found in VSX 2" Gaia DR3 134329916841955968
Type: ROT
# Max. Min./Amp. JD0 Period
12.630 G 12.650 G K
The object was not found in astcheck.
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:01.93 +32:56:09.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:01.93 +32:56:09.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 07 10.3333* 02 30 01.93 +32 56 09.1 11.9 U Tri 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 134329916841955968,2461231.8333,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134329916841955968 20260710.3333 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.06 02:35:20.65 +32:53:51.1
146.89194 -25.09471 galactic Tri Second-epoch detections are separated by 2.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:35:20.65 +32:53:51.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.461+/-0.028 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:20.65 +32:53:51.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:20.65 +32:53:51.1: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 35 20.65 +32 53 51.1 12.1 U Tri 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,2461231.8333,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.83 02:30:11.94 +33:17:06.7
145.63178 -25.19638 galactic Tri Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:30:11.94 +33:17:06.7 (user input) | T | P | (position from user input) J-Ks=0.591+/-0.027 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:11.94 +33:17:06.7: 12.81 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:11.94 +33:17:06.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 30 11.94 +33 17 06.7 11.8 U Tri 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,2461231.8333,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.77 02:44:42.62 +34:27:45.9
148.04123 -22.82687 galactic Tri Second-epoch detections are separated by 1.9" and 8.5 pix
The object was found in VSX 3" ASASSN-V J024442.80+342743.4
Type: L
# Max. Min./Amp. JD0 Period
13.490 V 13.980 V
The object was not found in astcheck.
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:44:42.62 +34:27:45.9: 12.81 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:44:42.62 +34:27:45.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 07 10.3333* 02 44 42.62 +34 27 45.9 11.8 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024442.80+342743.4,2461231.8333,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J024442.80+342743.4 20260710.3333 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.97 02:40:33.06 +34:01:22.7
147.42282 -23.60744 galactic Tri Second-epoch detections are separated by 0.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J040.1336+34.0110 | 02:40:33.06 +34:01:22.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:40:33.06 +34:01:22.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:40:33.06 +34:01:22.7: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 40 33.06 +34 01 22.7 12.0 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J040.1336+34.0110,2461231.8333,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J040.1336+34.0110 20260710.3333 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.84 02:37:41.67 +32:32:32.7
147.55434 -25.19931 galactic Tri Second-epoch detections are separated by 1.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:37:41.67 +32:32:32.7 (user input) | T | P | (position from user input) J-Ks=0.644+/-0.032 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:41.67 +32:32:32.7: 12.79 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:41.67 +32:32:32.7: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 37 41.67 +32 32 32.7 11.8 U Tri 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,2461231.8333,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.84 02:37:38.89 +33:11:29.0
147.23076 -24.62041 galactic Tri Second-epoch detections are separated by 0.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:37:38.89 +33:11:29.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.636+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:38.89 +33:11:29.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:38.89 +33:11:29.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 37 38.89 +33 11 29.0 11.8 U Tri 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,2461231.8333,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.80 02:31:17.35 +33:53:32.1
145.58421 -24.54969 galactic Tri Second-epoch detections are separated by 1.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:31:17.35 +33:53:32.1 (user input) | T | P | (position from user input) J-Ks=0.641+/-0.027 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:17.35 +33:53:32.1: 12.77 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:17.35 +33:53:32.1: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 31 17.35 +33 53 32.1 11.8 U Tri 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,2461231.8333,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.83 02:32:43.87 +32:43:55.4
146.42060 -25.47833 galactic Tri Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 134211818125004928 | 02:32:43.86 +32:43:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.857+/-0.027 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:43.87 +32:43:55.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:43.87 +32:43:55.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 32 43.87 +32 43 55.4 11.8 U Tri 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 134211818125004928,2461231.8333,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134211818125004928 20260710.3333 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.99 02:46:12.62 +34:19:07.7
148.41115 -22.81202 galactic Tri Second-epoch detections are separated by 1.9" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:46:12.62 +34:19:07.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.317+/-0.031 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:46:12.62 +34:19:07.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:46:12.62 +34:19:07.7: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 46 12.62 +34 19 07.7 12.0 U Tri 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,2461231.8333,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.02 02:36:33.54 +33:09:48.6
147.01839 -24.74482 galactic Tri Second-epoch detections are separated by 1.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:33.54 +33:09:48.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:33.54 +33:09:48.6: 13.00 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:33.54 +33:09:48.6: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 07 10.3333* 02 36 33.54 +33 09 48.6 12.0 U Tri 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,2461231.8333,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.91 02:32:14.77 +34:08:48.0
145.66666 -24.23599 galactic Tri Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:14.77 +34:08:48.0 (user input) | T | P | (position from user input) J-Ks=0.745+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:14.77 +34:08:48.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:14.77 +34:08:48.0: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 07 10.3333* 02 32 14.77 +34 08 48.0 11.9 U Tri 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,2461231.8333,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.90 02:29:35.22 +32:43:50.3
145.75442 -25.75471 galactic Tri Second-epoch detections are separated by 4.0" and 8.1 pix
The object was found in VSX 0" Gaia DR3 134317925293352192
Type: RS
# Max. Min./Amp. JD0 Period
12.760 G 12.820 G K
The object was not found in astcheck.
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:35.22 +32:43:50.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:35.22 +32:43:50.3: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 29 35.22 +32 43 50.3 11.9 U Tri 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 134317925293352192,2461231.8333,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134317925293352192 20260710.3333 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.01 02:32:04.93 +33:11:12.3
146.07280 -25.12279 galactic Tri Second-epoch detections are separated by 1.9" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:04.93 +33:11:12.3 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.028 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:04.93 +33:11:12.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:04.93 +33:11:12.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 32 04.93 +33 11 12.3 12.0 U Tri 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,2461231.8333,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.72 02:36:35.14 +33:28:30.4
146.87535 -24.46159 galactic Tri Second-epoch detections are separated by 2.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1427+33.4625 | 02:36:35.16 +33:28:29.9 (Gaia DR3) | SINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.096+/-0.027 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:35.14 +33:28:30.4: 12.70 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:35.14 +33:28:30.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 36 35.14 +33 28 30.4 11.7 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.1427+33.4625,2461231.8333,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.1427+33.4625 20260710.3333 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.19 02:41:13.31 +33:15:27.9
147.93401 -24.22930 galactic Tri Second-epoch detections are separated by 5.2" and 9.4 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 | 02:41:13.31 +33:15:27.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:13.31 +33:15:27.9: 13.20 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:13.31 +33:15:27.9: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 41 13.31 +33 15 27.9 12.2 U Tri 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,2461231.8333,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.09 02:32:07.97 +33:26:39.1
145.96478 -24.88445 galactic Tri Second-epoch detections are separated by 3.9" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.0325+33.4435 | 02:32:07.97 +33:26:39.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:07.97 +33:26:39.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:07.97 +33:26:39.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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 07 10.3333* 02 32 07.97 +33 26 39.1 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0325+33.4435,2461231.8333,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0325+33.4435 20260710.3333 12.09CV 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 07 10.3333 2461231.8333 11.94 02:33:56.71 +32:51:57.6
146.61355 -25.24892 galactic Tri Second-epoch detections are separated by 0.9" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4862+32.8658 | 02:33:56.71 +32:51:57.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.862+/-0.026 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:56.71 +32:51:57.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:56.71 +32:51:57.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 33 56.71 +32 51 57.6 11.9 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4862+32.8658,2461231.8333,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4862+32.8658 20260710.3333 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.96 02:41:54.67 +34:01:48.0
147.69430 -23.47505 galactic Tri Second-epoch detections are separated by 1.4" and 9.1 pix
The object was found in VSX 0" Gaia DR3 134724297920277632
Type: ROT
# Max. Min./Amp. JD0 Period
12.740 G 12.760 G K
The object was not found in astcheck.
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:54.67 +34:01:48.0: 12.95 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:54.67 +34:01:48.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 07 10.3333* 02 41 54.67 +34 01 48.0 12.0 U Tri 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 134724297920277632,2461231.8333,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134724297920277632 20260710.3333 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.17 02:34:42.62 +32:58:52.8
146.71960 -25.07609 galactic Tri Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:34:42.62 +32:58:52.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.515+/-0.030 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:42.62 +32:58:52.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:42.62 +32:58:52.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 34 42.62 +32 58 52.8 12.2 U Tri 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,2461231.8333,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.90 02:29:33.56 +33:09:17.2
145.55595 -25.37017 galactic Tri Second-epoch detections are separated by 5.2" 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 | 02:29:33.56 +33:09:17.2 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:33.56 +33:09:17.2: 12.94 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:33.56 +33:09:17.2: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 07 10.3333* 02 29 33.56 +33 09 17.2 11.9 U Tri 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,2461231.8333,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.69 02:41:20.82 +32:40:24.0
148.24936 -24.73907 galactic Tri Second-epoch detections are separated by 1.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 133742262239365120 | 02:41:20.84 +32:40:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.034+/-0.027 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:20.82 +32:40:24.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:20.82 +32:40:24.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 41 20.82 +32 40 24.0 11.7 U Tri 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 133742262239365120,2461231.8333,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 133742262239365120 20260710.3333 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.01 02:31:11.21 +32:49:06.7
146.05386 -25.53575 galactic Tri Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:31:11.21 +32:49:06.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.466+/-0.029 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:11.21 +32:49:06.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:11.21 +32:49:06.7: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 31 11.21 +32 49 06.7 12.0 U Tri 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,2461231.8333,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.82 02:30:35.92 +32:50:25.4
145.91919 -25.56710 galactic Tri Second-epoch detections are separated by 0.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 134325312636160384 | 02:30:35.77 +32:50:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:35.92 +32:50:25.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:35.92 +32:50:25.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 07 10.3333* 02 30 35.92 +32 50 25.4 11.8 U Tri 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 134325312636160384,2461231.8333,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134325312636160384 20260710.3333 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.95 02:43:35.70 +33:21:18.7
148.36953 -23.91747 galactic Tri Second-epoch detections are separated by 2.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:43:35.70 +33:21:18.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.865+/-0.028 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:43:35.70 +33:21:18.7: 12.92 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:43:35.70 +33:21:18.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 43 35.70 +33 21 18.7 11.9 U Tri 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,2461231.8333,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.66 02:32:26.74 +34:10:43.5
145.69318 -24.18965 galactic Tri Second-epoch detections are separated by 1.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 134916471938588544 | 02:32:26.76 +34:10:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:26.74 +34:10:43.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:26.74 +34:10:43.5: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 32 26.74 +34 10 43.5 11.7 U Tri 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 134916471938588544,2461231.8333,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134916471938588544 20260710.3333 11.66CV 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 07 10.3333 2461231.8333 12.22 02:34:08.32 +34:34:39.2
145.85761 -23.68123 galactic Tri Second-epoch detections are separated by 2.5" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:34:08.32 +34:34:39.2 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.582+/-0.029 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:08.32 +34:34:39.2: 13.22 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:08.32 +34:34:39.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 07 10.3333* 02 34 08.32 +34 34 39.2 12.2 U Tri 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,2461231.8333,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.62 02:35:16.66 +32:34:46.2
147.02947 -25.38773 galactic Tri Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 134140212431467776 | 02:35:16.72 +32:34:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.784+/-0.027 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:16.66 +32:34:46.2: 12.57 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:16.66 +32:34:46.2: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 35 16.66 +32 34 46.2 11.6 U Tri 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 134140212431467776,2461231.8333,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134140212431467776 20260710.3333 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.96 02:33:27.92 +34:28:00.5
145.77091 -23.83999 galactic Tri Second-epoch detections are separated by 2.1" and 8.3 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 | 02:33:27.92 +34:28:00.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.495+/-0.033 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:27.92 +34:28:00.5: 12.91 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:27.92 +34:28:00.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 33 27.92 +34 28 00.5 12.0 U Tri 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,2461231.8333,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.12 02:32:30.39 +34:47:15.1
145.42901 -23.63068 galactic Tri Second-epoch detections are separated by 2.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:30.39 +34:47:15.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.556+/-0.032 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:30.39 +34:47:15.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:30.39 +34:47:15.1: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 07 10.3333* 02 32 30.39 +34 47 15.1 12.1 U Tri 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,2461231.8333,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.93 02:37:27.78 +33:13:38.7
147.17512 -24.60494 galactic Tri Second-epoch detections are separated by 2.4" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:37:27.78 +33:13:38.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.490+/-0.027 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:27.78 +33:13:38.7: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:27.78 +33:13:38.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 37 27.78 +33 13 38.7 11.9 U Tri 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,2461231.8333,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.88 02:29:48.02 +32:40:07.8
145.82806 -25.79262 galactic Tri Second-epoch detections are separated by 0.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 134316550903759360 | 02:29:48.86 +32:39:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.320+/-0.030 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:48.02 +32:40:07.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:48.02 +32:40:07.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 29 48.02 +32 40 07.8 11.9 U Tri 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 134316550903759360,2461231.8333,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 134316550903759360 20260710.3333 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.20 02:37:00.61 +33:11:42.9
147.09678 -24.67519 galactic Tri Second-epoch detections are separated by 5.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:37:00.61 +33:11:42.9 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.850+/-0.027 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:00.61 +33:11:42.9: 13.43 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:00.61 +33:11:42.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 37 00.61 +33 11 42.9 12.2 U Tri 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,2461231.8333,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.20CV 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 07 10.3333 2461231.8333 12.13 02:35:47.86 +32:51:13.7
147.00763 -25.09309 galactic Tri Second-epoch detections are separated by 3.4" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:35:47.86 +32:51:13.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.270+/-0.031 (F)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:47.86 +32:51:13.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:47.86 +32:51:13.7: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 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!
TCP 2026 07 10.3333* 02 35 47.86 +32 51 13.7 12.1 U Tri 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,2461231.8333,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.10 02:41:36.11 +33:16:12.3
148.00568 -24.18250 galactic Tri Second-epoch detections are separated by 1.7" and 8.5 pix
The object was found in VSX 2" Gaia DR3 133913270655122048
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.180 G 13.210 G A
The object was not found in astcheck.
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:36.11 +33:16:12.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:36.11 +33:16:12.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 41 36.11 +33 16 12.3 12.1 U Tri 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 133913270655122048,2461231.8333,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 133913270655122048 20260710.3333 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.19 02:35:36.53 +33:12:49.6
146.79703 -24.78538 galactic Tri Second-epoch detections are separated by 1.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:35:36.53 +33:12:49.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.436+/-0.028 (G)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:36.53 +33:12:49.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:36.53 +33:12:49.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 07 10.3333* 02 35 36.53 +33 12 49.6 12.2 U Tri 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,2461231.8333,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.04 02:32:42.31 +34:02:48.9
145.80700 -24.28709 galactic Tri Second-epoch detections are separated by 1.3" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:42.31 +34:02:48.9 (user input) | T | P | (position from user input) J-Ks=0.669+/-0.026 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:42.31 +34:02:48.9: 13.18 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:42.31 +34:02:48.9: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 32 42.31 +34 02 48.9 12.0 U Tri 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,2461231.8333,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.96 02:32:16.89 +33:55:12.9
145.77735 -24.43884 galactic Tri Second-epoch detections are separated by 1.3" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:16.89 +33:55:12.9 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:16.89 +33:55:12.9: 12.88 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:16.89 +33:55:12.9: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 32 16.89 +33 55 12.9 12.0 U Tri 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,2461231.8333,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.86 02:31:27.11 +33:14:18.5
145.91662 -25.13071 galactic Tri Second-epoch detections are separated by 2.5" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:31:27.11 +33:14:18.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:27.11 +33:14:18.5: 12.88 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:27.11 +33:14:18.5: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 31 27.11 +33 14 18.5 11.9 U Tri 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,2461231.8333,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 12.02 02:29:28.89 +32:56:34.1
145.63552 -25.57026 galactic Tri Second-epoch detections are separated by 3.9" and 8.2 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 | 02:29:28.89 +32:56:34.1 (user input) | T | P | (position from user input) J-Ks=0.562+/-0.028 (K)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:28.89 +32:56:34.1: 13.15 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:28.89 +32:56:34.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 29 28.89 +32 56 34.1 12.0 U Tri 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,2461231.8333,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260710.3333 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.3333 2461231.8333 11.86 02:43:15.00 +32:25:28.9
148.76724 -24.77758 galactic Tri Second-epoch detections are separated by 2.5" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 133539058743231488 | 02:43:15.00 +32:25:28.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.131+/-0.050 (M)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:43:15.00 +32:25:28.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:43:15.00 +32:25:28.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 10.3333* 02 43 15.00 +32 25 28.9 11.9 U Tri 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 133539058743231488,2461231.8333,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 133539058743231488 20260710.3333 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.72860486 23.12.2025 05:29:01.460 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
First image: 2461032.72860486 23.12.2025 05:29:01.460 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Last image: 2461231.83362550 10.07.2026 08:00:15.243 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17290
Objects passed selection criteria: 17158
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: 9759.5
Average stars matched: 9496.75 (97.3078 %)
Memory usage VmPeak: 122164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 04:01:17 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.72860486 23.12.2025 05:29:01.460 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
First image: 2461032.72860486 23.12.2025 05:29:01.460 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Last image: 2461231.83362550 10.07.2026 08:00:15.243 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 83
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 104632
Objects passed selection criteria: 104223
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 60980.5
Average stars matched: 58629.8 (96.1451 %)
Memory usage VmPeak: 1936408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 10 04:05:19 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
SExtractor catalog cache: saved And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.cat to cache
SExtractor catalog cache: saved And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.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/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.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: 2461231.83290949
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'
Plate-solving the images
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits exists and is non-empty
Saving wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits to local_wcs_cache/
'wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits' -> 'local_wcs_cache/wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits'
wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits exists and is non-empty
Saving wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits to local_wcs_cache/
'wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits' -> 'local_wcs_cache/wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits'
wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits exists and is non-empty
Saving wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits to local_wcs_cache/
'wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits' -> 'local_wcs_cache/wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits'
wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits exists and is non-empty
Saving wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits to local_wcs_cache/
'wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits' -> 'local_wcs_cache/wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits (1st reference image)
verification OK: wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Image size: 941.4'x626.9' 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: 02:10:53.294 +38:00:08.11 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_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits (1st new image)
verification OK: wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:11:06.974 +37:59:46.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:10:53.294 +38:00:08.11
Second-epoch image center 02:11:06.974 +37:59:46.13
Angular distance between the image centers 0.0453 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits (2nd new image)
verification OK: wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:11:04.637 +37:59:04.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:10:53.294 +38:00:08.11
Second-epoch image center 02:11:04.637 +37:59:04.85
Angular distance between the image centers 0.0412 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 02:11:06.974 +37:59:46.13
Second-epoch second image center 02:11:04.637 +37:59:04.85
Angular distance between the image centers 0.01380 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/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits &> /tmp/tmp.FzevEOZKQx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits &> /tmp/tmp.LjrdcnmERZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits &> /tmp/tmp.pa03HI1lTa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits &> /tmp/tmp.3X03yeuCBj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.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_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits and wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.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_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits and wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
Found non-empty wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits and wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
The reference image (wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits) and catalog (wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat) found
'wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat' -> 'wcsmag.cat'
Read 18523 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 22.2405 to 43.6004 deg, Dec +32.1878 to +43.3127 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 22.2405 to 43.6004 deg, Dec 32.1878 to 43.3127 deg
Loaded 13070 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): 9333 out of 10127 total matches.
Matched with Tycho-2 10127 out of 18523 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929000
a=0.000000 b=1.000000 c=22.929000
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18523 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 22.2405 to 43.6004 deg, Dec +32.1878 to +43.3127 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 22.2405 to 43.6004 deg, Dec 32.1878 to 43.3127 deg
Loaded 13070 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): 9333 out of 10127 total matches.
Matched with Tycho-2 10127 out of 18523 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits:
Forced-photometry filter: calibrated wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits -> calib.txt_param_ref_wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits (aperture=6.0)
Read 18408 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 22.2834 to 43.6148 deg, Dec +32.1877 to +43.3132 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 22.2834 to 43.6148 deg, Dec 32.1877 to 43.3132 deg
Loaded 13051 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): 9281 out of 10101 total matches.
Matched with Tycho-2 10101 out of 18408 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits:
Forced-photometry filter: calibrated wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits -> calib.txt_param_ref_wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits (aperture=6.0)
____ 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:
2.0 pix And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
2.0 pix And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
3.3 pix fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
3.1 pix fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
2.0 pix wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
2.0 pix wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Limiting magnitude estimates:
15.4 mag. And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
15.4 mag. And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
13.1 mag. fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
12.0 mag. fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 10.2 (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
############ /tmp/tmp.FzevEOZKQx (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits' -> 'wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
WCS_IMAGE_NAME=wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
WCS-calibrated image found: wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Checking if the catalog wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits alredy exist and is non-empty...
Catalog wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
WCS catalog name: wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1587, bad_region=0, passed=18523
Got 18523 stars (including 16914 good ones) from the SExtractor catalog wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
util/solve_plate_with_UCAC5 got 18523 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 18019 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 18017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 18017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits N_match=951 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.254 n_q1=231 n_q2=275 n_q3=196 n_q4=249 worst_quadrant_to_overall_ratio=1.256
The image catalog is written to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits -region wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LjrdcnmERZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits' -> 'wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
WCS-calibrated image found: wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Checking if the catalog wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
WCS catalog name: wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1621, bad_region=0, passed=18408
Got 18408 stars (including 16764 good ones) from the SExtractor catalog wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat
util/solve_plate_with_UCAC5 got 18408 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 18041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 18042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 18042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits N_match=954 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.320 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.292 n_q1=238 n_q2=266 n_q3=202 n_q4=248 worst_quadrant_to_overall_ratio=1.059
The image catalog is written to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits -region wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pa03HI1lTa (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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
WCS_IMAGE_NAME=wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
WCS-calibrated image found: wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Checking if the catalog wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
WCS catalog name: wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=42, bad_region=0, passed=1102
Got 1102 stars (including 1059 good ones) from the SExtractor catalog wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 1102 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 1026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 1027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 1027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 932 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits N_match=932 sigma_overall_arcsec=0.507 sigma_q1_arcsec=0.683 sigma_q2_arcsec=0.502 sigma_q3_arcsec=0.553 sigma_q4_arcsec=0.481 n_q1=81 n_q2=486 n_q3=162 n_q4=203 worst_quadrant_to_overall_ratio=1.347
The image catalog is written to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits -region wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3X03yeuCBj (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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
WCS_IMAGE_NAME=wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
WCS-calibrated image found: wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Checking if the catalog wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
WCS catalog name: wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=37, bad_region=0, passed=1220
Got 1220 stars (including 1182 good ones) from the SExtractor catalog wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat
util/solve_plate_with_UCAC5 got 1220 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 1135 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 1136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 1136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits N_match=929 sigma_overall_arcsec=0.458 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.464 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.436 n_q1=83 n_q2=397 n_q3=184 n_q4=265 worst_quadrant_to_overall_ratio=1.039
The image catalog is written to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits -region wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits sigma_overall=0.339 worst_q_ratio=1.256
ref2=And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits sigma_overall=0.362 worst_q_ratio=1.059
new1=fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits sigma_overall=0.507 worst_q_ratio=1.347
new2=fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits sigma_overall=0.458 worst_q_ratio=1.039
reference average sigma_overall=0.3505 worst_q_ratio=1.1575
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241_astrometric_residuals.png (951 matched stars from wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124_astrometric_residuals.png (954 matched stars from wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300_astrometric_residuals.png (932 matched stars from wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301_astrometric_residuals.png (929 matched stars from wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits'
Saving fully-calibrated image wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits'
Preparing the HTML report for the field And-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field And-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
SExtractor catalog cache: saved And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.cat to cache
SExtractor catalog cache: saved And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Creating symlink local_wcs_cache/wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Creating symlink local_wcs_cache/wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Creating symlink local_wcs_cache/wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits exists and is non-empty
wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits exists and is non-empty
wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits exists and is non-empty
wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits (1st reference image)
verification OK: wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Image size: 941.4'x626.9' 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: 02:10:53.294 +38:00:08.11 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_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits (1st new image)
verification OK: wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:11:06.974 +37:59:46.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:10:53.294 +38:00:08.11
Second-epoch image center 02:11:06.974 +37:59:46.13
Angular distance between the image centers 0.0453 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits (2nd new image)
verification OK: wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Image size: 942.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:11:04.637 +37:59:04.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:10:53.294 +38:00:08.11
Second-epoch image center 02:11:04.637 +37:59:04.85
Angular distance between the image centers 0.0412 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 02:11:06.974 +37:59:46.13
Second-epoch second image center 02:11:04.637 +37:59:04.85
Angular distance between the image centers 0.01380 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/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits &> /tmp/tmp.azkYLRjuKW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits &> /tmp/tmp.zInkOBJjCK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits &> /tmp/tmp.DJqzYADQ2X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits &> /tmp/tmp.Y7z6bTe2dt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.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_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits and wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.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_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits and wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
Found non-empty wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits and wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
The reference image (wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits) and catalog (wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat) found
'wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat' -> 'wcsmag.cat'
Read 113384 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 22.2164 to 43.6004 deg, Dec +32.1473 to +43.3244 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 22.2164 to 43.6004 deg, Dec 32.1473 to 43.3244 deg
Loaded 13140 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): 8005 out of 10343 total matches.
Matched with Tycho-2 10343 out of 113384 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.813200
a=0.000000 b=1.000000 c=22.813200
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 113384 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 22.2164 to 43.6004 deg, Dec +32.1473 to +43.3244 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 22.2164 to 43.6004 deg, Dec 32.1473 to 43.3244 deg
Loaded 13140 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): 8005 out of 10343 total matches.
Matched with Tycho-2 10343 out of 113384 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits:
Forced-photometry filter: calibrated wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits -> calib.txt_param_ref_wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits (aperture=4.7)
Read 114316 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 22.2703 to 43.6315 deg, Dec +32.1472 to +43.3169 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 22.2703 to 43.6315 deg, Dec 32.1472 to 43.3169 deg
Loaded 13111 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): 7970 out of 10336 total matches.
Matched with Tycho-2 10336 out of 114316 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits:
Forced-photometry filter: calibrated wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits -> calib.txt_param_ref_wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 74 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
1.9 pix And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
2.9 pix fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
2.8 pix fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
1.9 pix wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
1.9 pix wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Limiting magnitude estimates:
15.5 mag. And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
15.5 mag. And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
12.4 mag. fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
12.4 mag. fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 11.9 (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.azkYLRjuKW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits' -> 'wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
WCS_IMAGE_NAME=wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
WCS-calibrated image found: wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
Checking if the catalog wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits alredy exist and is non-empty...
Catalog wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits
WCS catalog name: wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=10724, bad_region=9, passed=113353
Got 113353 stars (including 102434 good ones) from the SExtractor catalog wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat
util/solve_plate_with_UCAC5 got 113353 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 110763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 110763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 110763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits N_match=959 sigma_overall_arcsec=0.337 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.266 n_q1=229 n_q2=272 n_q3=198 n_q4=260 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits -region wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zInkOBJjCK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits' -> 'wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
WCS-calibrated image found: wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
Checking if the catalog wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat corresponding to the image wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits
WCS catalog name: wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=10865, bad_region=9, passed=114291
Got 114291 stars (including 103221 good ones) from the SExtractor catalog wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat
util/solve_plate_with_UCAC5 got 114291 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 112274 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 112274 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 112273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits N_match=962 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.303 n_q1=224 n_q2=274 n_q3=207 n_q4=257 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits -region wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DJqzYADQ2X (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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
WCS_IMAGE_NAME=wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
WCS-calibrated image found: wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Checking if the catalog wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
WCS catalog name: wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=174, bad_region=3, passed=8260
Got 8260 stars (including 8070 good ones) from the SExtractor catalog wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 8260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 7521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 7522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 7522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits N_match=926 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.624 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.525 sigma_q4_arcsec=0.477 n_q1=84 n_q2=462 n_q3=174 n_q4=206 worst_quadrant_to_overall_ratio=1.268
The image catalog is written to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits -region wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Y7z6bTe2dt (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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
WCS_IMAGE_NAME=wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
WCS-calibrated image found: wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Checking if the catalog wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat corresponding to the image wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
WCS catalog name: wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=232, bad_region=3, passed=9564
Got 9564 stars (including 9305 good ones) from the SExtractor catalog wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat
util/solve_plate_with_UCAC5 got 9564 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 8677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 8667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits N_match=927 sigma_overall_arcsec=0.439 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.409 n_q1=84 n_q2=386 n_q3=189 n_q4=268 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits -region wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/wcs_fd_And-06-Q1b1x1_2026-07-10_02-59-13_20.00sec_-0.00C_LIGHTs_0300.fits
Saving fully-calibrated image wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.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_2026-07-10_CI_And-06-Q1b1x1_031355_TTUQ1b1x1_3571421_L8rV4UQz/wcs_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301.fits
Preparing the HTML report for the field And-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:47:23.43 +34:17:39.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:45:48.73 +32:15:51.4: 12.56 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:38.90 +32:51:31.7: 12.70 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:46:13.38 +32:30:48.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:46.91 +42:22:20.8: 12.76 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:39.20 +33:02:02.2: 13.13 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:47:23.43 +34:17:39.8: 12.80 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:40:40.34 +34:14:35.1: 12.50 +/- 0.01 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:03.68 +32:37:34.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:45:48.73 +32:15:51.4: 12.46 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 02:47:23.43 +34:17:39.8: ref_mag=12.83 +/- 0.02 new_mean_mag=12.0829 delta=0.75 (need > 0.90)
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:38.90 +32:51:31.7: 12.64 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 02:45:48.73 +32:15:51.4: ref_mag=12.51 +/- 0.01 new_mean_mag=11.7467 delta=0.76 (need > 0.90)
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter REJECTED candidate at 02:35:38.90 +32:51:31.7: ref_mag=12.67 +/- 0.01 new_mean_mag=11.7889 delta=0.88 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:03.83 +32:43:36.4: 13.13 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:46:13.38 +32:30:48.5: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter REJECTED candidate at 02:46:13.38 +32:30:48.5: ref_mag=12.89 +/- 0.02 new_mean_mag=12.0956 delta=0.80 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:46.91 +42:22:20.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:46.91 +42:22:20.8: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8670 delta=0.91 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:39.20 +33:02:02.2: 13.10 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:40:40.34 +34:14:35.1: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:00.08 +42:34:00.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:03.68 +32:37:34.9: 13.14 +/- 0.03 detection
Forced photometry filter KEPT candidate at 02:36:39.20 +33:02:02.2: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1243 delta=0.99 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:40:40.34 +34:14:35.1: ref_mag=12.50 +/- 0.01 new_mean_mag=11.6062 delta=0.89 (need > 0.90)
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 02:36:03.68 +32:37:34.9: ref_mag=13.15 +/- 0.02 new_mean_mag=12.0923 delta=1.06 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:03.83 +32:43:36.4: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 02:35:03.83 +32:43:36.4: ref_mag=13.12 +/- 0.02 new_mean_mag=12.0638 delta=1.06 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:00.08 +42:34:00.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 02:34:00.08 +42:34:00.3: ref_mag=13.04 +/- 0.02 new_mean_mag=11.9871 delta=1.05 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:38:34.73 +34:14:21.3: 13.09 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:52.71 +33:12:52.0: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:46.78 +32:39:13.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:40:48.85 +33:38:35.2: 13.08 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:37.29 +33:16:34.6: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:38:34.73 +34:14:21.3: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 02:38:34.73 +34:14:21.3: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0368 delta=1.03 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:52.71 +33:12:52.0: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 02:35:52.71 +33:12:52.0: ref_mag=13.00 +/- 0.02 new_mean_mag=11.9964 delta=1.00 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:46.78 +32:39:13.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:46.78 +32:39:13.0: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8861 delta=0.97 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:40:48.85 +33:38:35.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 02:40:48.85 +33:38:35.2: ref_mag=13.08 +/- 0.02 new_mean_mag=12.0133 delta=1.06 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:37.29 +33:16:34.6: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 02:30:37.29 +33:16:34.6: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0243 delta=1.02 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:39:05.59 +33:54:14.3: 12.84 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:16.33 +33:05:46.6: 13.06 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:19.51 +32:42:27.0: 12.83 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:42:07.47 +34:02:06.3: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:39:05.59 +33:54:14.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 02:39:05.59 +33:54:14.3: ref_mag=12.83 +/- 0.01 new_mean_mag=11.8762 delta=0.95 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:16.33 +33:05:46.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 02:35:16.33 +33:05:46.6: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0508 delta=0.94 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:19.51 +32:42:27.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:19.51 +32:42:27.0: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8884 delta=0.97 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:42:07.47 +34:02:06.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 02:42:07.47 +34:02:06.3: ref_mag=13.04 +/- 0.02 new_mean_mag=11.9782 delta=1.06 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:02.51 +33:46:11.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:37.88 +32:45:31.5: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:47.79 +33:50:43.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:28.54 +33:26:50.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:14.64 +33:11:12.3: 12.83 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:37.88 +32:45:31.5: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 02:30:37.88 +32:45:31.5: ref_mag=13.08 +/- 0.02 new_mean_mag=11.9886 delta=1.09 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:47.79 +33:50:43.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:12.12 +34:25:31.3: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:28.54 +33:26:50.6: 13.07 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:02.51 +33:46:11.7: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 02:31:47.79 +33:50:43.0: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0004 delta=1.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:14.64 +33:11:12.3: 12.81 +/- 0.02 detection
Forced photometry filter KEPT candidate at 02:31:02.51 +33:46:11.7: ref_mag=13.07 +/- 0.02 new_mean_mag=11.9484 delta=1.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 02:31:28.54 +33:26:50.6: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0489 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:14.64 +33:11:12.3: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7961 delta=1.03 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:12.12 +34:25:31.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:12.12 +34:25:31.3: ref_mag=13.00 +/- 0.01 new_mean_mag=12.0443 delta=0.96 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:46.96 +32:50:45.9: 13.05 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:01.93 +32:56:09.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:20.65 +32:53:51.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:46.96 +32:50:45.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 02:34:46.96 +32:50:45.9: ref_mag=13.07 +/- 0.02 new_mean_mag=11.8841 delta=1.18 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:01.93 +32:56:09.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 02:30:01.93 +32:56:09.1: ref_mag=12.99 +/- 0.02 new_mean_mag=11.8843 delta=1.11 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:20.65 +32:53:51.1: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 02:35:20.65 +32:53:51.1: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0521 delta=1.00 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:11.94 +33:17:06.7: 12.81 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:11.94 +33:17:06.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:11.94 +33:17:06.7: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8229 delta=0.98 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:44:42.62 +34:27:45.9: 12.81 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:40:33.06 +34:01:22.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:44:42.62 +34:27:45.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 02:44:42.62 +34:27:45.9: ref_mag=12.83 +/- 0.02 new_mean_mag=11.7596 delta=1.07 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:41.67 +32:32:32.7: 12.79 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:40:33.06 +34:01:22.7: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 02:40:33.06 +34:01:22.7: ref_mag=13.02 +/- 0.02 new_mean_mag=11.9761 delta=1.04 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:17.35 +33:53:32.1: 12.77 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:41.67 +32:32:32.7: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 02:37:41.67 +32:32:32.7: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8289 delta=0.93 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:38.89 +33:11:29.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:17.35 +33:53:32.1: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:17.35 +33:53:32.1: ref_mag=12.74 +/- 0.01 new_mean_mag=11.7844 delta=0.96 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:38.89 +33:11:29.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 02:37:38.89 +33:11:29.0: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8379 delta=0.93 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:43.87 +32:43:55.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:46:12.62 +34:19:07.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:43.87 +32:43:55.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 02:32:43.87 +32:43:55.4: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8289 delta=0.93 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:46:12.62 +34:19:07.7: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 02:46:12.62 +34:19:07.7: ref_mag=12.98 +/- 0.02 new_mean_mag=11.9761 delta=1.01 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:33.54 +33:09:48.6: 13.00 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:33.54 +33:09:48.6: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 02:36:33.54 +33:09:48.6: ref_mag=12.99 +/- 0.02 new_mean_mag=11.9499 delta=1.04 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:14.77 +34:08:48.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:35.22 +32:43:50.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:04.93 +33:11:12.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:14.77 +34:08:48.0: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 02:32:14.77 +34:08:48.0: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9303 delta=1.02 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:35.22 +32:43:50.3: 12.91 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:04.93 +33:11:12.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:35.22 +32:43:50.3: ref_mag=12.94 +/- 0.01 new_mean_mag=11.9048 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 02:32:04.93 +33:11:12.3: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9880 delta=0.91 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:36:35.14 +33:28:30.4: 12.70 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:36:35.14 +33:28:30.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 02:36:35.14 +33:28:30.4: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7104 delta=0.99 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:13.31 +33:15:27.9: 13.20 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:07.97 +33:26:39.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:13.31 +33:15:27.9: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 02:41:13.31 +33:15:27.9: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1802 delta=1.01 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:07.97 +33:26:39.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 02:32:07.97 +33:26:39.1: ref_mag=13.25 +/- 0.02 new_mean_mag=12.0912 delta=1.16 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:56.71 +32:51:57.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:54.67 +34:01:48.0: 12.95 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:56.71 +32:51:57.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:56.71 +32:51:57.6: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9291 delta=0.97 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:42.62 +32:58:52.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:54.67 +34:01:48.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 02:41:54.67 +34:01:48.0: ref_mag=12.91 +/- 0.02 new_mean_mag=11.9365 delta=0.97 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:42.62 +32:58:52.8: 13.25 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:33.56 +33:09:17.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 02:34:42.62 +32:58:52.8: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1427 delta=1.09 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:20.82 +32:40:24.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:33.56 +33:09:17.2: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:33.56 +33:09:17.2: ref_mag=12.92 +/- 0.01 new_mean_mag=11.8777 delta=1.04 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:20.82 +32:40:24.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 02:41:20.82 +32:40:24.0: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6835 delta=0.95 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:11.21 +32:49:06.7: 12.93 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:11.21 +32:49:06.7: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:11.21 +32:49:06.7: ref_mag=12.93 +/- 0.01 new_mean_mag=12.0122 delta=0.92 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:35.92 +32:50:25.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:43:35.70 +33:21:18.7: 12.92 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:35.92 +32:50:25.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 02:30:35.92 +32:50:25.4: ref_mag=12.92 +/- 0.01 new_mean_mag=11.8200 delta=1.10 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:43:35.70 +33:21:18.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 02:43:35.70 +33:21:18.7: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9467 delta=0.98 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:26.74 +34:10:43.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:26.74 +34:10:43.5: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 02:32:26.74 +34:10:43.5: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6600 delta=0.94 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:34:08.32 +34:34:39.2: 13.22 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:34:08.32 +34:34:39.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 02:34:08.32 +34:34:39.2: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2029 delta=1.02 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:16.66 +32:34:46.2: 12.57 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:33:27.92 +34:28:00.5: 12.91 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:16.66 +32:34:46.2: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 02:35:16.66 +32:34:46.2: ref_mag=12.57 +/- 0.01 new_mean_mag=11.5950 delta=0.97 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:33:27.92 +34:28:00.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 02:33:27.92 +34:28:00.5: ref_mag=12.91 +/- 0.01 new_mean_mag=11.9565 delta=0.96 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:30.39 +34:47:15.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:30.39 +34:47:15.1: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter KEPT candidate at 02:32:30.39 +34:47:15.1: ref_mag=13.41 +/- 0.02 new_mean_mag=12.1153 delta=1.29 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:27.78 +33:13:38.7: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:27.78 +33:13:38.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 02:37:27.78 +33:13:38.7: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9232 delta=0.97 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:48.02 +32:40:07.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:48.02 +32:40:07.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 02:29:48.02 +32:40:07.8: ref_mag=12.88 +/- 0.01 new_mean_mag=11.8845 delta=1.00 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:30:57.62 +33:23:29.7: 12.52 +/- 0.01 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:30:57.62 +33:23:29.7: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter REJECTED candidate at 02:30:57.62 +33:23:29.7: ref_mag=12.50 +/- 0.01 new_mean_mag=11.6467 delta=0.85 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:37:00.61 +33:11:42.9: 13.43 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:37:00.61 +33:11:42.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 02:37:00.61 +33:11:42.9: ref_mag=13.39 +/- 0.02 new_mean_mag=12.1752 delta=1.22 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:47.86 +32:51:13.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:47.86 +32:51:13.7: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 02:35:47.86 +32:51:13.7: ref_mag=13.15 +/- 0.02 new_mean_mag=12.1290 delta=1.02 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:36.11 +33:16:12.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:36.11 +33:16:12.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 02:41:36.11 +33:16:12.3: ref_mag=13.19 +/- 0.02 new_mean_mag=12.0506 delta=1.14 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:35:36.53 +33:12:49.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:42.31 +34:02:48.9: 13.18 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:35:36.53 +33:12:49.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 02:35:36.53 +33:12:49.6: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1524 delta=1.02 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:42.31 +34:02:48.9: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 02:32:42.31 +34:02:48.9: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0336 delta=1.11 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:32:16.89 +33:55:12.9: 12.88 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:31:27.11 +33:14:18.5: 12.88 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:32:16.89 +33:55:12.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:41:16.86 +33:51:28.0: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 02:32:16.89 +33:55:12.9: ref_mag=12.88 +/- 0.01 new_mean_mag=11.9386 delta=0.95 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:31:27.11 +33:14:18.5: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 02:31:27.11 +33:14:18.5: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8293 delta=1.03 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:41:16.86 +33:51:28.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 02:41:16.86 +33:51:28.0: ref_mag=12.46 +/- 0.01 new_mean_mag=11.5641 delta=0.89 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:29:28.89 +32:56:34.1: 13.15 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:29:28.89 +32:56:34.1: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 02:29:28.89 +32:56:34.1: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0499 delta=1.09 (need > 0.90)
Forced photometry on wcs_And-06-Q1b1x1_2025-12-22_23-29-01_20.00sec_-15.00C_LIGHT_0241.fits at 02:43:15.00 +32:25:28.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_And-06-Q1b1x1_2026-01-08_21-54-17_20.00sec_-15.00C_LIGHT_0124.fits at 02:43:15.00 +32:25:28.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 02:43:15.00 +32:25:28.9: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8656 delta=0.98 (need > 0.90)
Adding exclusion_list_local.txt__out05795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93625.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 96s
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 132485_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 132485_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 132487_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 132487_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 132571_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 132571_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 132582_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 132582_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 02:32:09.23 +36:10:41.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 132637_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 132637_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 78750_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78750_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 08454_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 08454_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 88819_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 88819_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
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Considering the candidate 79328_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 79328_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 81858_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 81858_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 05795_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 05795_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 88236_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 88236_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 78640_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78640_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 83094_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 83094_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 85653_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 85653_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 82860_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82860_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 82125_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82125_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 83968_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 83968_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 78484_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78484_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 86397_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 86397_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 88790_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 88790_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 106954_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 106954_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 84960_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 84960_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 79007_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 79007_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 82006_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82006_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 89194_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 89194_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 80130_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 80130_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 80202_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 80202_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 80608_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 80608_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 82874_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82874_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 92830_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 92830_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 85968_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 85968_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 78395_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78395_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 83159_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 83159_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 111992_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 111992_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 79069_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 79069_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 92008_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 92008_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 82823_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82823_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 85262_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 85262_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 78690_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78690_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 82373_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82373_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 103630_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 103630_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 107675_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 107675_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 106662_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 106662_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 80175_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 80175_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 86341_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 86341_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 81157_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 81157_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 81809_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 81809_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 79858_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 79858_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 79514_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 79514_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 79586_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 79586_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 108262_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 108262_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
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Considering the candidate 85762_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 85762_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91499_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 91499_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95070_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 95070_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 02:46:56.73 +34:34:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78337_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78337_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89917_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 89917_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93625_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 93625_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83407_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 83407_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78211_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78211_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87651_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 87651_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 02:37:02.32 +34:15:52.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111149_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 111149_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83103_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 83103_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80348_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 80348_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105669_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 105669_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83055_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 83055_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84490_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 84490_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93339_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 93339_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82585_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 82585_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84082_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 84082_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92204_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 92204_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 02:09:33.03 +34:59:17.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80172_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 80172_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09587_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
The candidate 09587_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301 did not pass the final checks
**** FOUND 02:03:54.22 +42:19:41.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78384_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
Preparing report for the candidate 78384_fd_And-06-Q1b1x1_2026-07-10_03-00-15_20.00sec_0.00C_LIGHTs_0301
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 144s
Prepared the HTML report for the field And-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:34:00.08 +42:34:00.3
02:33:46.91 +42:22:20.8
02:36:35.14 +33:28:30.4
02:41:36.11 +33:16:12.3
02:32:07.97 +33:26:39.1
02:31:28.54 +33:26:50.6
02:41:13.31 +33:15:27.9
02:43:35.70 +33:21:18.7
02:31:17.35 +33:53:32.1
02:29:48.02 +32:40:07.8
02:35:16.66 +32:34:46.2
02:43:15.00 +32:25:28.9
02:37:41.67 +32:32:32.7
02:29:19.51 +32:42:27.0
02:33:46.78 +32:39:13.0
02:29:35.22 +32:43:50.3
02:36:03.68 +32:37:34.9
02:30:37.88 +32:45:31.5
02:32:43.87 +32:43:55.4
02:35:03.83 +32:43:36.4
02:31:11.21 +32:49:06.7
02:30:35.92 +32:50:25.4
02:41:20.82 +32:40:24.0
02:34:46.96 +32:50:45.9
02:29:28.89 +32:56:34.1
02:33:56.71 +32:51:57.6
02:30:01.93 +32:56:09.1
02:35:47.86 +32:51:13.7
02:35:20.65 +32:53:51.1
02:34:42.62 +32:58:52.8
02:29:33.56 +33:09:17.2
02:36:39.20 +33:02:02.2
02:29:14.64 +33:11:12.3
02:35:16.33 +33:05:46.6
02:32:04.93 +33:11:12.3
02:31:27.11 +33:14:18.5
02:36:33.54 +33:09:48.6
02:30:37.29 +33:16:34.6
02:30:11.94 +33:17:06.7
02:35:36.53 +33:12:49.6
02:35:52.71 +33:12:52.0
02:37:00.61 +33:11:42.9
02:37:38.89 +33:11:29.0
02:37:27.78 +33:13:38.7
02:39:05.59 +33:54:14.3
02:32:42.31 +34:02:48.9
02:31:47.79 +33:50:43.0
02:32:14.77 +34:08:48.0
02:40:48.85 +33:38:35.2
02:32:26.74 +34:10:43.5
02:40:33.06 +34:01:22.7
02:41:54.67 +34:01:48.0
02:42:07.47 +34:02:06.3
02:38:34.73 +34:14:21.3
02:31:02.51 +33:46:11.7
02:33:12.12 +34:25:31.3
02:33:27.92 +34:28:00.5
02:34:08.32 +34:34:39.2
02:46:12.62 +34:19:07.7
02:44:42.62 +34:27:45.9
02:32:16.89 +33:55:12.9
02:32:30.39 +34:47:15.1
########### Completed And-06-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
02:36:03.68 +32:37:34.9
02:33:46.91 +42:22:20.8
02:35:03.83 +32:43:36.4
02:36:39.20 +33:02:02.2
02:34:00.08 +42:34:00.3
02:38:34.73 +34:14:21.3
02:33:46.78 +32:39:13.0
02:35:52.71 +33:12:52.0
02:40:48.85 +33:38:35.2
02:30:37.29 +33:16:34.6
02:35:16.33 +33:05:46.6
02:39:05.59 +33:54:14.3
02:29:19.51 +32:42:27.0
02:42:07.47 +34:02:06.3
02:31:02.51 +33:46:11.7
02:31:28.54 +33:26:50.6
02:31:47.79 +33:50:43.0
02:30:37.88 +32:45:31.5
02:29:14.64 +33:11:12.3
02:33:12.12 +34:25:31.3
02:34:46.96 +32:50:45.9
02:30:01.93 +32:56:09.1
02:35:20.65 +32:53:51.1
02:30:11.94 +33:17:06.7
02:44:42.62 +34:27:45.9
02:40:33.06 +34:01:22.7
02:37:41.67 +32:32:32.7
02:37:38.89 +33:11:29.0
02:31:17.35 +33:53:32.1
02:32:43.87 +32:43:55.4
02:46:12.62 +34:19:07.7
02:36:33.54 +33:09:48.6
02:32:14.77 +34:08:48.0
02:29:35.22 +32:43:50.3
02:32:04.93 +33:11:12.3
02:36:35.14 +33:28:30.4
02:41:13.31 +33:15:27.9
02:32:07.97 +33:26:39.1
02:33:56.71 +32:51:57.6
02:41:54.67 +34:01:48.0
02:34:42.62 +32:58:52.8
02:29:33.56 +33:09:17.2
02:41:20.82 +32:40:24.0
02:31:11.21 +32:49:06.7
02:30:35.92 +32:50:25.4
02:43:35.70 +33:21:18.7
02:32:26.74 +34:10:43.5
02:34:08.32 +34:34:39.2
02:35:16.66 +32:34:46.2
02:33:27.92 +34:28:00.5
02:32:30.39 +34:47:15.1
02:37:27.78 +33:13:38.7
02:29:48.02 +32:40:07.8
02:37:00.61 +33:11:42.9
02:35:47.86 +32:51:13.7
02:41:36.11 +33:16:12.3
02:35:36.53 +33:12:49.6
02:32:42.31 +34:02:48.9
02:32:16.89 +33:55:12.9
02:31:27.11 +33:14:18.5
02:29:28.89 +32:56:34.1
02:43:15.00 +32:25:28.9
###################################################################################
02:36:03.68 +32:37:34.9 -- not an asteroid (will add it to exclusion list)
02:33:46.91 +42:22:20.8 -- not an asteroid (will add it to exclusion list)
02:35:03.83 +32:43:36.4 -- not an asteroid (will add it to exclusion list)
02:36:39.20 +33:02:02.2 -- not an asteroid (will add it to exclusion list)
02:34:00.08 +42:34:00.3 -- not an asteroid (will add it to exclusion list)
02:38:34.73 +34:14:21.3 -- not an asteroid (will add it to exclusion list)
02:33:46.78 +32:39:13.0 -- not an asteroid (will add it to exclusion list)
02:35:52.71 +33:12:52.0 -- not an asteroid (will add it to exclusion list)
02:40:48.85 +33:38:35.2 -- not an asteroid (will add it to exclusion list)
02:30:37.29 +33:16:34.6 -- not an asteroid (will add it to exclusion list)
02:35:16.33 +33:05:46.6 -- not an asteroid (will add it to exclusion list)
02:39:05.59 +33:54:14.3 -- not an asteroid (will add it to exclusion list)
02:29:19.51 +32:42:27.0 -- not an asteroid (will add it to exclusion list)
02:42:07.47 +34:02:06.3 -- not an asteroid (will add it to exclusion list)
02:31:02.51 +33:46:11.7 -- not an asteroid (will add it to exclusion list)
02:31:28.54 +33:26:50.6 -- not an asteroid (will add it to exclusion list)
02:31:47.79 +33:50:43.0 -- not an asteroid (will add it to exclusion list)
02:30:37.88 +32:45:31.5 -- not an asteroid (will add it to exclusion list)
02:29:14.64 +33:11:12.3 -- not an asteroid (will add it to exclusion list)
02:33:12.12 +34:25:31.3 -- not an asteroid (will add it to exclusion list)
02:34:46.96 +32:50:45.9 -- not an asteroid (will add it to exclusion list)
02:30:01.93 +32:56:09.1 -- not an asteroid (will add it to exclusion list)
02:35:20.65 +32:53:51.1 -- not an asteroid (will add it to exclusion list)
02:30:11.94 +33:17:06.7 -- not an asteroid (will add it to exclusion list)
02:44:42.62 +34:27:45.9 -- not an asteroid (will add it to exclusion list)
02:40:33.06 +34:01:22.7 -- not an asteroid (will add it to exclusion list)
02:37:41.67 +32:32:32.7 -- not an asteroid (will add it to exclusion list)
02:37:38.89 +33:11:29.0 -- not an asteroid (will add it to exclusion list)
02:31:17.35 +33:53:32.1 -- not an asteroid (will add it to exclusion list)
02:32:43.87 +32:43:55.4 -- not an asteroid (will add it to exclusion list)
02:46:12.62 +34:19:07.7 -- not an asteroid (will add it to exclusion list)
02:36:33.54 +33:09:48.6 -- not an asteroid (will add it to exclusion list)
02:32:14.77 +34:08:48.0 -- not an asteroid (will add it to exclusion list)
02:29:35.22 +32:43:50.3 -- not an asteroid (will add it to exclusion list)
02:32:04.93 +33:11:12.3 -- not an asteroid (will add it to exclusion list)
02:36:35.14 +33:28:30.4 -- not an asteroid (will add it to exclusion list)
02:41:13.31 +33:15:27.9 -- not an asteroid (will add it to exclusion list)
02:32:07.97 +33:26:39.1 -- not an asteroid (will add it to exclusion list)
02:33:56.71 +32:51:57.6 -- not an asteroid (will add it to exclusion list)
02:41:54.67 +34:01:48.0 -- not an asteroid (will add it to exclusion list)
02:34:42.62 +32:58:52.8 -- not an asteroid (will add it to exclusion list)
02:29:33.56 +33:09:17.2 -- not an asteroid (will add it to exclusion list)
02:41:20.82 +32:40:24.0 -- not an asteroid (will add it to exclusion list)
02:31:11.21 +32:49:06.7 -- not an asteroid (will add it to exclusion list)
02:30:35.92 +32:50:25.4 -- not an asteroid (will add it to exclusion list)
02:43:35.70 +33:21:18.7 -- not an asteroid (will add it to exclusion list)
02:32:26.74 +34:10:43.5 -- not an asteroid (will add it to exclusion list)
02:34:08.32 +34:34:39.2 -- not an asteroid (will add it to exclusion list)
02:35:16.66 +32:34:46.2 -- not an asteroid (will add it to exclusion list)
02:33:27.92 +34:28:00.5 -- not an asteroid (will add it to exclusion list)
02:32:30.39 +34:47:15.1 -- not an asteroid (will add it to exclusion list)
02:37:27.78 +33:13:38.7 -- not an asteroid (will add it to exclusion list)
02:29:48.02 +32:40:07.8 -- not an asteroid (will add it to exclusion list)
02:37:00.61 +33:11:42.9 -- not an asteroid (will add it to exclusion list)
02:35:47.86 +32:51:13.7 -- not an asteroid (will add it to exclusion list)
02:41:36.11 +33:16:12.3 -- not an asteroid (will add it to exclusion list)
02:35:36.53 +33:12:49.6 -- not an asteroid (will add it to exclusion list)
02:32:42.31 +34:02:48.9 -- not an asteroid (will add it to exclusion list)
02:32:16.89 +33:55:12.9 -- not an asteroid (will add it to exclusion list)
02:31:27.11 +33:14:18.5 -- not an asteroid (will add it to exclusion list)
02:29:28.89 +32:56:34.1 -- not an asteroid (will add it to exclusion list)
02:43:15.00 +32:25:28.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
02:29:14.64 +33:11:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:19.51 +32:42:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:28.89 +32:56:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:33.56 +33:09:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:35.22 +32:43:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:48.02 +32:40:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:01.93 +32:56:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:11.94 +33:17:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:35.92 +32:50:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:37.29 +33:16:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:37.88 +32:45:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:02.51 +33:46:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:11.21 +32:49:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:17.35 +33:53:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:27.11 +33:14:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:28.54 +33:26:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:47.79 +33:50:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.93 +33:11:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:07.97 +33:26:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:14.77 +34:08:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:16.89 +33:55:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:26.74 +34:10:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:30.39 +34:47:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:42.31 +34:02:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:43.87 +32:43:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:12.12 +34:25:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:27.92 +34:28:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:46.78 +32:39:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:46.91 +42:22:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:56.71 +32:51:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:00.08 +42:34:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:08.32 +34:34:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:42.62 +32:58:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:46.96 +32:50:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:03.83 +32:43:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:16.33 +33:05:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:16.66 +32:34:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:20.65 +32:53:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:36.53 +33:12:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:47.86 +32:51:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:52.71 +33:12:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:03.68 +32:37:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:33.54 +33:09:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:35.14 +33:28:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:39.20 +33:02:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:00.61 +33:11:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:27.78 +33:13:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:38.89 +33:11:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:41.67 +32:32:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:34.73 +34:14:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:05.59 +33:54:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:40:33.06 +34:01:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:40:48.85 +33:38:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:13.31 +33:15:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:20.82 +32:40:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:36.11 +33:16:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:54.67 +34:01:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:42:07.47 +34:02:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:43:15.00 +32:25:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:43:35.70 +33:21:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:44:42.62 +34:27:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:46:12.62 +34:19:07.7 -- 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)
02:29:14.64 +33:11:12.3 -- not a known variable star
02:29:19.51 +32:42:27.0 -- not a known variable star
02:29:28.89 +32:56:34.1 -- not a known variable star
02:29:33.56 +33:09:17.2 -- not a known variable star
02:29:35.22 +32:43:50.3 -- a known variable star
02:29:48.02 +32:40:07.8 -- not a known variable star
02:30:01.93 +32:56:09.1 -- a known variable star
02:30:11.94 +33:17:06.7 -- not a known variable star
02:30:35.92 +32:50:25.4 -- not a known variable star
02:30:37.29 +33:16:34.6 -- not a known variable star
02:30:37.88 +32:45:31.5 -- not a known variable star
02:31:02.51 +33:46:11.7 -- not a known variable star
02:31:11.21 +32:49:06.7 -- not a known variable star
02:31:17.35 +33:53:32.1 -- not a known variable star
02:31:27.11 +33:14:18.5 -- not a known variable star
02:31:28.54 +33:26:50.6 -- not a known variable star
02:31:47.79 +33:50:43.0 -- not a known variable star
02:32:04.93 +33:11:12.3 -- not a known variable star
02:32:07.97 +33:26:39.1 -- not a known variable star
02:32:14.77 +34:08:48.0 -- not a known variable star
02:32:16.89 +33:55:12.9 -- not a known variable star
02:32:26.74 +34:10:43.5 -- not a known variable star
02:32:30.39 +34:47:15.1 -- not a known variable star
02:32:42.31 +34:02:48.9 -- not a known variable star
02:32:43.87 +32:43:55.4 -- not a known variable star
02:33:12.12 +34:25:31.3 -- not a known variable star
02:33:27.92 +34:28:00.5 -- not a known variable star
02:33:46.78 +32:39:13.0 -- not a known variable star
02:33:46.91 +42:22:20.8 -- not a known variable star
02:33:56.71 +32:51:57.6 -- not a known variable star
02:34:00.08 +42:34:00.3 -- not a known variable star
02:34:08.32 +34:34:39.2 -- not a known variable star
02:34:42.62 +32:58:52.8 -- not a known variable star
02:34:46.96 +32:50:45.9 -- not a known variable star
02:35:03.83 +32:43:36.4 -- not a known variable star
02:35:16.33 +33:05:46.6 -- not a known variable star
02:35:16.66 +32:34:46.2 -- not a known variable star
02:35:20.65 +32:53:51.1 -- not a known variable star
02:35:36.53 +33:12:49.6 -- not a known variable star
02:35:47.86 +32:51:13.7 -- not a known variable star
02:35:52.71 +33:12:52.0 -- not a known variable star
02:36:03.68 +32:37:34.9 -- not a known variable star
02:36:33.54 +33:09:48.6 -- not a known variable star
02:36:35.14 +33:28:30.4 -- not a known variable star
02:36:39.20 +33:02:02.2 -- not a known variable star
02:37:00.61 +33:11:42.9 -- not a known variable star
02:37:27.78 +33:13:38.7 -- not a known variable star
02:37:38.89 +33:11:29.0 -- not a known variable star
02:37:41.67 +32:32:32.7 -- not a known variable star
02:38:34.73 +34:14:21.3 -- not a known variable star
02:39:05.59 +33:54:14.3 -- not a known variable star
02:40:33.06 +34:01:22.7 -- not a known variable star
02:40:48.85 +33:38:35.2 -- not a known variable star
02:41:13.31 +33:15:27.9 -- not a known variable star
02:41:20.82 +32:40:24.0 -- not a known variable star
02:41:36.11 +33:16:12.3 -- a known variable star
02:41:54.67 +34:01:48.0 -- a known variable star
02:42:07.47 +34:02:06.3 -- not a known variable star
02:43:15.00 +32:25:28.9 -- not a known variable star
02:43:35.70 +33:21:18.7 -- not a known variable star
02:44:42.62 +34:27:45.9 -- a known variable star
02:46:12.62 +34:19:07.7 -- not a known variable star
Found 57 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
62 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 62 (excluding asteroids and hot pixels, 57 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)2461231.83290949 -observatory V36
07:32:19.46 +17:08:03.8 Mercury (5.1mag)
10:11:34.27 +12:41:27.7 Venus (-4.1mag)
04:24:07.17 +21:25:04.1 Mars (1.3mag)
08:16:39.59 +20:11:32.0 Jupiter (-1.8mag)
00:55:50.79 +03:20:28.4 Saturn (0.7mag)
04:07:13.83 +20:45:02.8 Uranus (5.8mag)
00:17:01.50 +00:20:41.3 Neptune (7.8mag)
20:30:55.04 -23:18:00.1 Pluto (14.4mag)
03:10:37.01 +22:14:27.1 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 361 Jul 10 04:01 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461231.83290949:
08:16:46.08 +20:11:09.6 Io (6.1mag)
08:16:42.14 +20:11:24.4 Europa (6.3mag)
08:16:56.61 +20:10:30.6 Ganymede (5.6mag)
08:17:07.64 +20:09:48.4 Callisto (6.8mag)
08:15:11.13 +19:55:41.2 Himalia (15.7mag)
08:16:38.44 +20:11:37.3 Thebe (16.6mag)
08:14:32.47 +20:00:11.0 Elara (17.6mag)
08:20:11.78 +20:05:42.7 Pasiphae (17.8mag)
08:21:37.50 +20:16:36.9 Carme (19.0mag)
00:55:40.61 +03:20:19.5 Titan (8.5mag)
00:55:45.55 +03:20:31.7 Rhea (9.8mag)
00:55:20.11 +03:19:37.5 Iapetus (11.2mag)
00:56:00.09 +03:20:47.4 Hyperion (14.5mag)
00:55:51.54 +03:17:42.4 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 10 04:01 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461231.83290949:
17:46:10.22 -32:59:54.6 JWST
16:12:18.09 +49:08:43.9 Chandra
02:04:41.62 +63:32:42.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 10 04:01 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461231.83290949 -observatory V36
02:36:14.58 +14:25:33.7 17.9mag P/1996 R2 (Lagerkvist)
18:17:57.26 -34:21:43.6 13.7mag P/2010 H2 (Vales)
06:25:39.35 -68:08:22.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:00:47.98 +32:26:47.9 17.6mag C/2017 K2 (PANSTARRS)
17:03:07.28 +16:02:54.8 18.0mag C/2021 G2 (ATLAS)
01:47:41.92 +08:10:59.3 15.4mag P/2021 N1 (ZTF)
22:59:32.55 +32:17:08.0 17.3mag C/2022 E2 (ATLAS)
06:12:22.68 +26:55:35.2 16.7mag C/2022 N2 (PANSTARRS)
09:55:29.92 +29:46:54.2 16.8mag C/2022 QE78 (ATLAS)
09:09:43.38 +04:59:55.9 17.8mag C/2022 R6 (PANSTARRS)
18:07:13.78 +21:17:40.5 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:35.35 -11:23:14.5 17.7mag P/2023 B1 (PANSTARRS)
21:49:15.45 +67:37:17.0 17.8mag C/2023 H5 (Lemmon)
16:30:55.38 -10:04:34.5 13.9mag C/2023 R1 (PANSTARRS)
08:00:37.06 +65:42:26.7 17.9mag C/2024 A1 (ATLAS)
07:32:47.37 +30:00:08.5 14.6mag C/2024 E1 (Wierzchos)
15:16:20.12 +15:19:40.2 17.5mag C/2024 G6 (ATLAS)
19:41:20.03 +39:23:21.6 13.8mag C/2024 J3 (ATLAS)
21:47:36.13 +46:00:01.4 17.8mag C/2024 R4 (PANSTARRS)
04:49:37.28 -13:47:48.4 15.7mag C/2024 T5 (ATLAS)
06:34:33.44 +29:04:22.8 18.0mag C/2025 J1 (Borisov)
07:14:19.53 -12:53:16.8 16.5mag C/2025 R3 (PANSTARRS)
09:56:04.18 +22:26:15.6 17.6mag C/2025 V2 (Rankin)
12:44:36.64 +03:56:19.0 17.1mag C/2025 Y1 (ATLAS)
16:52:00.49 +79:07:11.8 17.4mag C/2026 A2 (Bok)
02:46:15.32 +45:14:20.3 16.7mag C/2026 B2 (Sun-Gao)
11:25:29.94 +04:32:26.6 16.9mag A/2026 E1
21:19:00.50 -15:04:11.0 7.3mag 10P/Tempel
11:13:26.76 -01:53:11.0 16.1mag 29P/Schwassmann-Wachmann
04:00:08.67 +29:33:03.8 17.8mag 47P/Ashbrook-Jackson
10:08:02.16 +14:01:03.2 17.0mag 63P/Wild
00:48:21.24 -05:05:36.1 15.5mag 65P/Gunn
08:26:53.55 +34:13:11.0 17.9mag 76P/West-Kohoutek-Ikemura
04:27:21.08 +20:10:39.8 13.7mag 78P/Gehrels
02:22:18.17 +10:36:24.5 16.2mag 88P/Howell
06:35:28.35 +30:32:09.1 15.7mag 93P/Lovas
04:20:56.19 +31:07:19.6 16.9mag 114P/Wiseman-Skiff
08:08:38.81 +30:42:20.3 15.3mag 123P/West-Hartley
10:48:05.70 +01:11:41.3 16.8mag 124P/Mrkos
04:51:41.81 +20:48:44.6 16.2mag 128P/Shoemaker-Holt
05:36:13.13 +19:42:51.0 17.8mag 131P/Mueller
00:01:32.41 +02:56:04.1 17.9mag 139P/Vaisala-Oterma
07:13:29.37 +17:01:29.5 15.5mag 141P-D/Machholz
03:16:50.44 -21:06:27.1 15.5mag 161P/Hartley-IRAS
05:32:59.61 +33:56:39.6 15.3mag 162P/SidingSpring
19:04:31.37 +15:04:15.1 14.7mag 169P/NEAT
01:40:59.03 +07:35:47.1 17.7mag 220P/McNaught
16:35:58.32 -08:23:04.7 17.0mag 235P/LINEAR
08:45:14.66 +33:18:04.4 17.9mag 240P/NEAT
20:42:11.04 -49:33:58.7 17.8mag 259P/Garradd
01:59:15.14 +12:05:08.4 15.7mag 260P/McNaught
05:37:10.02 +36:50:28.7 17.4mag 295P/LINEAR
15:06:36.86 +06:03:31.0 17.6mag 391P/Kowalski
08:34:35.16 +19:40:39.2 17.9mag 450P/LONEOS
07:51:44.15 +39:13:04.0 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 10 04:01 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 10 04:01 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:36:21.258 +13:42:31.91 AT 2026sqg 2026-07-06.96 17.376
10:38:47.961 +53:30:34.10 SN 2026sqf 2026-07-08.25 12.9
13:40:20.447 +40:38:15.61 AT 2026sqe 2026-07-03.20 20.3209
20:26:11.475 -21:05:59.62 AT 2026sqd 2026-07-07.33 20.2909
20:38:05.960 -15:39:19.94 AT 2026sqc 2026-07-07.33 22.2834
21:50:20.218 -14:25:11.02 AT 2026sqb 2026-07-07.39 21.5547
20:32:17.644 -16:37:51.49 AT 2026sqa 2026-07-07.33 21.6569
20:38:02.144 -16:39:15.94 AT 2026spz 2026-07-07.33 22.7762
20:36:24.191 -15:13:43.37 AT 2026spy 2026-07-07.33 22.1739
20:41:10.988 -25:49:45.49 AT 2026spx 2026-07-07.33 22.8645
21:17:15.336 -23:31:53.39 AT 2026spw 2026-07-07.32 21.9459
20:27:45.431 -19:59:58.81 AT 2026spv 2026-07-07.33 21.6485
21:55:34.604 -14:11:57.66 AT 2026spu 2026-07-07.39 23.0585
21:10:34.181 -22:59:24.76 AT 2026spt 2026-07-07.32 22.3526
21:05:55.405 -19:04:02.26 AT 2026sps 2026-07-07.32 21.4424
20:59:14.423 -27:33:25.12 AT 2026spr 2026-07-07.32 23.4151
20:31:34.503 -19:06:25.71 AT 2026spq 2026-07-07.33 22.7105
20:54:43.024 -26:43:41.99 AT 2026spp 2026-07-07.32 22.8017
21:07:49.748 -22:55:35.56 AT 2026spo 2026-07-07.32 22.494
20:57:55.962 -26:08:04.97 AT 2026spn 2026-07-07.32 22.7486
-rw-r--r-- 1 apache apache 30K Jul 10 04:01 tns_transients_list.txt
