This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.10 00:16:37.95 -26:52:53.7
32.77228 -82.24500 galactic Scl Second-epoch detections are separated by 0.5" and 9.9 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 | 00:16:37.95 -26:52:53.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:16:37.95 -26:52:53.7: 11.05 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:16:37.95 -26:52:53.7: 11.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3692 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.08 00:28:01.07 -28:16:52.5
19.04079 -84.69018 galactic Scl Second-epoch detections are separated by 4.2" and 10.4 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 | 00:28:01.07 -28:16:52.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:28:01.07 -28:16:52.5: 11.16 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:28:01.07 -28:16:52.5: 11.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3692 10.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.31 00:13:23.62 -26:59:02.7
31.73773 -81.53061 galactic Scl Second-epoch detections are separated by 1.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2323137987817283584 | 00:13:23.58 -26:59:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1971AJ.....76..338S SB 76 J-Ks=0.055+/-0.032 (A)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:13:23.62 -26:59:02.7: 11.23 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:13:23.62 -26:59:02.7: 11.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2323137987817283584,2461274.8692,10.31,0.05,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 2323137987817283584 20260822.3692 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.49 00:23:11.61 -27:47:41.2
25.23746 -83.70008 galactic Scl Second-epoch detections are separated by 1.2" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.24700 1990 VN5 102 -26 105 17.1 -0 -0
ATTENTION: measured mag 10.49 is 6.6 mag brighter than the predicted asteroid brightness 17.1 - the transient may be an unrelated new object!
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:23:11.61 -27:47:41.2: 11.53 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:23:11.61 -27:47:41.2: 11.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461274.8692,10.49,0.05,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
VARIABLE_NAME 20260822.3692 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.61 00:21:01.91 -27:12:39.3
30.49508 -83.23777 galactic Scl Second-epoch detections are separated by 1.8" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2322934303288287360 | 00:21:01.88 -27:12:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.029 (G)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:21:01.91 -27:12:39.3: 11.57 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:21:01.91 -27:12:39.3: 11.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2322934303288287360,2461274.8692,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2322934303288287360 20260822.3692 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.61 00:12:22.67 -26:48:02.7
32.86347 -81.29259 galactic Scl Second-epoch detections are separated by 0.9" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2335156435886883968 | 00:12:22.67 -26:48:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.264+/-0.033 (F)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:12:22.67 -26:48:02.7: 11.60 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:12:22.67 -26:48:02.7: 11.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2335156435886883968,2461274.8692,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2335156435886883968 20260822.3692 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.60 00:18:28.74 -27:35:38.8
27.39958 -82.66863 galactic Scl Second-epoch detections are separated by 1.9" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2322895786020495104 | 00:18:28.70 -27:35:37.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.571+/-0.032 (K)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:18:28.74 -27:35:38.8: 11.64 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:18:28.74 -27:35:38.8: 11.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2322895786020495104,2461274.8692,10.60,0.05,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 2322895786020495104 20260822.3692 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.62 00:22:58.55 -27:57:26.1
23.80901 -83.63764 galactic Scl Second-epoch detections are separated by 4.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2322085853972828672 | 00:22:58.63 -27:57:26.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:22:58.55 -27:57:26.1: 11.64 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:22:58.55 -27:57:26.1: 11.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2322085853972828672,2461274.8692,10.62,0.05,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 2322085853972828672 20260822.3692 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.65 00:18:36.88 -27:25:11.5
28.76356 -82.70197 galactic Scl Second-epoch detections are separated by 0.9" and 10.1 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 2322946569714613504 | 00:18:36.85 -27:25:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.281+/-0.031 (F)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:18:36.88 -27:25:11.5: 11.77 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:18:36.88 -27:25:11.5: 11.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2322946569714613504,2461274.8692,10.65,0.05,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 2322946569714613504 20260822.3692 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.77 00:17:53.54 -26:51:57.0
33.03341 -82.52425 galactic Scl Second-epoch detections are separated by 0.4" and 10.0 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 | 00:17:53.54 -26:51:57.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:53.54 -26:51:57.0: 12.15 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:53.54 -26:51:57.0: 12.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.77,0.05,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
target 20260822.3692 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.86 00:17:20.00 -26:45:11.9
33.81647 -82.39137 galactic Scl Second-epoch detections are separated by 2.2" and 10.1 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 | 00:17:20.00 -26:45:11.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:20.00 -26:45:11.9: 12.19 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:20.00 -26:45:11.9: 12.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.86,0.05,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 20260822.3692 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.56 00:26:15.63 -28:22:58.5
18.78370 -84.29109 galactic Scl Second-epoch detections are separated by 0.7" and 9.9 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 | 00:26:15.63 -28:22:58.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:26:15.63 -28:22:58.5: 11.94 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:26:15.63 -28:22:58.5: 11.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3692 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.64 00:13:55.53 -26:13:34.4
36.95304 -81.57382 galactic Scl Second-epoch detections are separated by 1.9" and 10.0 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 | 00:13:55.53 -26:13:34.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:13:55.53 -26:13:34.4: 11.88 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:13:55.53 -26:13:34.4: 11.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3692 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.66 23:56:53.77 -23:17:24.2
47.21721 -77.08868 galactic Cet Second-epoch detections are separated by 2.0" and 9.7 pix
The object was found in VSX 1" ASASSN-V J235653.72-231724.6
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 g Y 0.130 g 2458077.59400 1.000500000000
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:56:53.77 -23:17:24.2: 11.79 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:56:53.77 -23:17:24.2: 11.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3692* 23 56 53.77 -23 17 24.2 10.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235653.72-231724.6,2461274.8692,10.66,0.05,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
ASASSN-V J235653.72-231724.6 20260822.3692 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.57 00:15:12.52 -26:30:08.9
35.30311 -81.89426 galactic Scl Second-epoch detections are separated by 1.0" and 10.1 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 2323255017085785344 | 00:15:12.47 -26:30:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.435+/-0.030 (G)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:15:12.52 -26:30:08.9: 11.71 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:15:12.52 -26:30:08.9: 11.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2323255017085785344,2461274.8692,10.57,0.05,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 2323255017085785344 20260822.3692 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.54 00:14:12.57 -26:36:54.3
34.35410 -81.68393 galactic Scl Second-epoch detections are separated by 0.9" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2323247492303079168 | 00:14:12.56 -26:36:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.734+/-0.033 (K)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:14:12.57 -26:36:54.3: 11.59 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:14:12.57 -26:36:54.3: 11.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2323247492303079168,2461274.8692,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2323247492303079168 20260822.3692 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.47 23:53:29.41 -21:31:08.1
52.83478 -75.67005 galactic Aqr Second-epoch detections are separated by 2.7" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2341241756005995648 | 23:53:29.36 -21:31:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.361+/-0.031 (G)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:53:29.41 -21:31:08.1: 11.57 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:53:29.41 -21:31:08.1: 11.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2341241756005995648,2461274.8692,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2341241756005995648 20260822.3692 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.40 00:16:43.69 -26:51:39.5
32.93556 -82.26489 galactic Scl Second-epoch detections are separated by 2.1" and 10.1 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 | 00:16:43.69 -26:51:39.5 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.035 (G)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:16:43.69 -26:51:39.5: 11.51 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:16:43.69 -26:51:39.5: 11.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8692,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3692 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.25 00:15:54.86 -26:18:04.4
36.87234 -82.02581 galactic Scl Second-epoch detections are separated by 2.0" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2323281508444085248 | 00:15:54.80 -26:18:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.589+/-0.035 (K)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:15:54.86 -26:18:04.4: 11.28 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:15:54.86 -26:18:04.4: 11.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2323281508444085248,2461274.8692,10.25,0.05,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 2323281508444085248 20260822.3692 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.23 00:21:44.29 -27:58:58.5
23.82522 -83.36317 galactic Scl Second-epoch detections are separated by 0.3" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2322109016732214144 | 00:21:44.28 -27:58:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.660+/-0.033 (K)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:21:44.29 -27:58:58.5: 11.21 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:21:44.29 -27:58:58.5: 11.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2322109016732214144,2461274.8692,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2322109016732214144 20260822.3692 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.26 00:31:28.69 -28:33:41.6
13.78051 -85.36134 galactic Scl Second-epoch detections are separated by 2.9" and 10.0 pix
The object was found in VSX 1" Gaia DR3 2319132913633773568
Type: ROT
# Max. Min./Amp. JD0 Period
10.750 G 10.780 G K
The object was not found in astcheck.
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:31:28.69 -28:33:41.6: 11.18 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:31:28.69 -28:33:41.6: 11.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2319132913633773568,2461274.8692,10.26,0.05,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 2319132913633773568 20260822.3692 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3692 2461274.8692 10.21 00:27:04.31 -28:13:05.5
20.10470 -84.49696 galactic Scl Second-epoch detections are separated by 1.9" and 10.1 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 2322192717054868352 | 00:27:04.23 -28:13:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.032 (F)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:27:04.31 -28:13:05.5: 11.12 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:27:04.31 -28:13:05.5: 11.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2322192717054868352,2461274.8692,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2322192717054868352 20260822.3692 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 3
Ref. image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
First image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Last image: 2461274.86960106 22.08.2026 08:52:03.532 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.60
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: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 1727
Objects passed selection criteria: 1718
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 3
Average stars detected per image: 1236
Average stars matched: 1204.67 (97.4649 %)
Memory usage VmPeak: 228816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 03:58:37 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
First image: 2461228.89270660 07.07.2026 09:25:19.850 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Last image: 2461274.86960106 22.08.2026 08:52:03.532 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 10970
Objects passed selection criteria: 10931
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: 6419.5
Average stars matched: 6168 (96.0822 %)
Memory usage VmPeak: 237156 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 03:58:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
SExtractor catalog cache: saved Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.cat to cache
SExtractor catalog cache: saved Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
Last image: 2461274.86888543 22.08.2026 08:51:01.701 UTC
ERROR running VaST on the field Scl-01-Q1b1x1 (less than 4 images processed)
exp_start= 07.07.2026 09:25:19.850 exp= 20.000 JD= 2461228.89270660 ap= 6.4 rotation= 0.000 *detected= 1811 *matched= 1811 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
exp_start= 07.07.2026 09:26:13.935 exp= 20.000 JD= 2461228.89333258 ap= 6.3 rotation= -0.007 *detected= 1819 *matched= 1727 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
exp_start= 22.08.2026 08:51:01.701 exp= 20.000 JD= 2461274.86888543 ap= 5.4 rotation= 175.876 *detected= 70 *matched= 69 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
exp_start= 22.08.2026 08:52:03.532 exp= 20.000 JD= 2461274.86960106 ap= 5.5 rotation= 175.885 *detected= 78 *matched= 76 status=OK /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
SExtractor catalog cache: saved Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.cat to cache
SExtractor catalog cache: saved Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461274.86888543
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits exists and is non-empty
wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits exists and is non-empty
wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits exists and is non-empty
wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (1st reference image)
verification OK: wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Image size: 937.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:59:59.880 -25:59:51.98 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits (1st new image)
verification OK: wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
Image size: 941.2'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:55.487 -26:01:16.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:59.880 -25:59:51.98
Second-epoch image center 23:59:55.487 -26:01:16.75
Angular distance between the image centers 0.0287 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits (2nd new image)
verification OK: wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
Image size: 932.2'x627.7' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 23:59:58.491 -26:01:56.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:59.880 -25:59:51.98
Second-epoch image center 23:59:58.491 -26:01:56.73
Angular distance between the image centers 0.0350 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 23:59:55.487 -26:01:16.75
Second-epoch second image center 23:59:58.491 -26:01:56.73
Angular distance between the image centers 0.01581 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/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits &> /tmp/tmp.FT932OVrwb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits &> /tmp/tmp.kDZqLbiz6e
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits &> /tmp/tmp.6PI9u59RDK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits &> /tmp/tmp.1Ei5PJzi6E
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
Calibrating the magnitude scale
Found non-empty wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
Found non-empty wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits and wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
The reference image (wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits) and catalog (wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat) found
'wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 11986 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 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 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 deg
Loaded 4450 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): 3548 out of 3632 total matches.
Matched with Tycho-2 3632 out of 11986 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.120250
a=0.000000 b=1.000000 c=22.120250
From vast_summary.log: estimated ref. image limiting mag.: -8.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.81
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.81
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 11986 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 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 350.9560 to 9.1144 deg, Dec -31.2631 to -20.5314 deg
Loaded 4450 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): 3548 out of 3632 total matches.
Matched with Tycho-2 3632 out of 11986 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Forced-photometry filter: calibrated wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits -> calib.txt_param_ref_wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (aperture=4.9)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 12014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 350.9532 to 9.1191 deg, Dec -31.2609 to -20.5233 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 350.9532 to 9.1191 deg, Dec -31.2609 to -20.5233 deg
Loaded 4454 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): 3592 out of 3675 total matches.
Matched with Tycho-2 3675 out of 12014 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Forced-photometry filter: calibrated wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits -> calib.txt_param_ref_wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
2.1 pix Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
1.9 pix fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
1.8 pix fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
Limiting magnitude estimates:
13.8 mag. Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
13.8 mag. Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
10.8 mag. fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
11.0 mag. fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
All-image limiting magnitude estimate: 10.8 (SNR ) 10.7 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.FT932OVrwb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits' -> 'wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS-calibrated image found: wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
Checking if the catalog wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat corresponding to the image wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits
WCS catalog name: wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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=7, blended=392, bad_region=0, passed=11979
Got 11979 stars (including 11576 good ones) from the SExtractor catalog wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat
util/solve_plate_with_UCAC5 got 11979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.9560 through 0 to 9.1144, gap 9.1144 to 350.9560
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 11979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.9542 through 0 to 9.1163, gap 9.1163 to 350.9542
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 11979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4876 matched stars entering correct_measured_positions(), 11979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4876 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits N_match=4876 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.516 sigma_q3_arcsec=0.584 sigma_q4_arcsec=0.435 n_q1=1298 n_q2=1142 n_q3=1206 n_q4=1230 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits -region wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.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.kDZqLbiz6e (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits' -> 'wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
Checking if the catalog wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat corresponding to the image wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits
WCS catalog name: wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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=351, bad_region=0, passed=12012
Got 12012 stars (including 11639 good ones) from the SExtractor catalog wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat
util/solve_plate_with_UCAC5 got 12012 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.9532 through 0 to 9.1191, gap 9.1191 to 350.9532
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 12012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.9537 through 0 to 9.1184, gap 9.1184 to 350.9537
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 12012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 12012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits N_match=4873 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.440 sigma_q2_arcsec=0.472 sigma_q3_arcsec=0.563 sigma_q4_arcsec=0.448 n_q1=1308 n_q2=1151 n_q3=1198 n_q4=1216 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits -region wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.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.6PI9u59RDK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
WCS-calibrated image found: wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
WCS catalog name: wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.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=11, bad_region=1, passed=902
Got 902 stars (including 889 good ones) from the SExtractor catalog wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits.wcscat
util/solve_plate_with_UCAC5 got 902 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.7624 through 0 to 8.7577, gap 8.7577 to 350.7624
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.4 to -20.2)
Done reading UCAC5 zone files...
Matched 847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 847 matched stars entering correct_measured_positions(), 822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 847 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.7626 through 0 to 8.7579, gap 8.7579 to 350.7626
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.4 to -20.2)
Done reading UCAC5 zone files...
Matched 847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 847 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Accuracy estimation diagnostic: 847 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 847 stars left (next iteration limit 931)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 847 catalog matches do not cover the frame (367/216/256/8 per quadrant, need 52 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits N_match=847 sigma_overall_arcsec=0.767 sigma_q1_arcsec=0.795 sigma_q2_arcsec=0.829 sigma_q3_arcsec=0.704 sigma_q4_arcsec=1.950 n_q1=367 n_q2=216 n_q3=256 n_q4=8 worst_quadrant_to_overall_ratio=2.541
The image catalog is written to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits -region wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.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.1Ei5PJzi6E (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits.wcscat corresponding to the image wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.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=1, blended=7, bad_region=1, passed=979
Got 979 stars (including 970 good ones) from the SExtractor catalog wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits.wcscat
util/solve_plate_with_UCAC5 got 979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 932.2'
Seting catalog search parameters based on the expected field of view 932.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012947 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010358 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.5461 through 0 to 8.7600, gap 8.7600 to 351.5461
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.4 to -20.2)
Done reading UCAC5 zone files...
Matched 861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 844 matched stars entering correct_measured_positions(), 827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 839 matched stars entering correct_measured_positions(), 888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.97"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.5484 through 0 to 8.7586, gap 8.7586 to 351.5484
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.4 to -20.2)
Done reading UCAC5 zone files...
Matched 877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 872 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.37"
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.34"
Excluding outliers - 871 stars left (next iteration limit 922)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 871 catalog matches do not cover the frame (326/225/315/5 per quadrant, need 54 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits N_match=871 sigma_overall_arcsec=2.901 sigma_q1_arcsec=3.554 sigma_q2_arcsec=2.045 sigma_q3_arcsec=2.133 sigma_q4_arcsec=10.726 n_q1=326 n_q2=225 n_q3=315 n_q4=5 worst_quadrant_to_overall_ratio=3.697
The image catalog is written to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits -region wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.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_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-51-01_20.00sec_0.00C_LIGHTs_0092.fits'
Saving fully-calibrated image wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Scl-01-Q1b1x1_035245_TTUQ1b1x1_4059803_vsrMKA3s/wcs_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093.fits'
Preparing the HTML report for the field Scl-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:55:09.67 -21:23:27.3: 9.91 +/- 0.01 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:12:22.67 -26:48:02.7: 11.60 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:18:36.88 -27:25:11.5: 11.77 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:22:58.55 -27:57:26.1: 11.64 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:13:23.62 -26:59:02.7: 11.23 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:18:28.74 -27:35:38.8: 11.64 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:28:01.07 -28:16:52.5: 11.16 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:16:37.95 -26:52:53.7: 11.05 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:23:11.61 -27:47:41.2: 11.53 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:21:01.91 -27:12:39.3: 11.57 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:18:36.88 -27:25:11.5: 11.77 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:16:37.95 -26:52:53.7: 11.04 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:13:23.62 -26:59:02.7: 11.20 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:28:01.07 -28:16:52.5: 11.13 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:55:09.67 -21:23:27.3: 9.80 +/- 0.01 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:12:22.67 -26:48:02.7: 11.60 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:22:58.55 -27:57:26.1: 11.73 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:23:11.61 -27:47:41.2: 11.45 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:21:01.91 -27:12:39.3: 11.58 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:18:28.74 -27:35:38.8: 11.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Forced photometry filter KEPT candidate at 00:18:36.88 -27:25:11.5: ref_mag=11.77 +/- 0.02 new_mean_mag=10.6458 delta=1.13 (need > 0.90)
Forced photometry reference-image weighted average: 11.05 +/- 0.01
Forced photometry reference-image weighted average: 11.14 +/- 0.02
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Forced photometry filter KEPT candidate at 00:16:37.95 -26:52:53.7: ref_mag=11.05 +/- 0.01 new_mean_mag=10.1003 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 11.60 +/- 0.02
Forced photometry reference-image weighted average: 9.84 +/- 0.00
Forced photometry reference-image weighted average: 11.68 +/- 0.02
Forced photometry reference-image weighted average: 11.63 +/- 0.02
Forced photometry reference-image weighted average: 11.58 +/- 0.02
Forced photometry reference-image weighted average: 11.49 +/- 0.02
Forced photometry filter KEPT candidate at 00:28:01.07 -28:16:52.5: ref_mag=11.14 +/- 0.02 new_mean_mag=9.9982 delta=1.15 (need > 0.90)
Forced photometry filter KEPT candidate at 00:13:23.62 -26:59:02.7: ref_mag=11.21 +/- 0.01 new_mean_mag=10.2126 delta=1.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:55:09.67 -21:23:27.3: ref_mag=9.84 +/- 0.00 new_mean_mag=9.8270 delta=0.02 (need > 0.90)
Forced photometry filter KEPT candidate at 00:12:22.67 -26:48:02.7: ref_mag=11.60 +/- 0.02 new_mean_mag=10.6027 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 00:22:58.55 -27:57:26.1: ref_mag=11.68 +/- 0.02 new_mean_mag=10.5723 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 00:18:28.74 -27:35:38.8: ref_mag=11.63 +/- 0.02 new_mean_mag=10.5460 delta=1.09 (need > 0.90)
Forced photometry filter KEPT candidate at 00:21:01.91 -27:12:39.3: ref_mag=11.58 +/- 0.02 new_mean_mag=10.5511 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 00:23:11.61 -27:47:41.2: ref_mag=11.49 +/- 0.02 new_mean_mag=10.4899 delta=1.00 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:53.54 -26:51:57.0: 12.15 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:53.54 -26:51:57.0: 12.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.03
Forced photometry filter KEPT candidate at 00:17:53.54 -26:51:57.0: ref_mag=12.14 +/- 0.03 new_mean_mag=10.7525 delta=1.38 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:17:20.00 -26:45:11.9: 12.19 +/- 0.05 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:17:20.00 -26:45:11.9: 12.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Forced photometry filter KEPT candidate at 00:17:20.00 -26:45:11.9: ref_mag=12.17 +/- 0.03 new_mean_mag=10.8634 delta=1.31 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:26:15.63 -28:22:58.5: 11.94 +/- 0.04 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:26:15.63 -28:22:58.5: 11.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.03
Forced photometry filter KEPT candidate at 00:26:15.63 -28:22:58.5: ref_mag=11.92 +/- 0.03 new_mean_mag=10.5464 delta=1.38 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:13:55.53 -26:13:34.4: 11.88 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:13:55.53 -26:13:34.4: 11.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.02
Forced photometry filter KEPT candidate at 00:13:55.53 -26:13:34.4: ref_mag=11.85 +/- 0.02 new_mean_mag=10.5791 delta=1.27 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:56:53.77 -23:17:24.2: 11.79 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:56:53.77 -23:17:24.2: 11.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.02
Forced photometry filter KEPT candidate at 23:56:53.77 -23:17:24.2: ref_mag=11.81 +/- 0.02 new_mean_mag=10.6488 delta=1.16 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:15:12.52 -26:30:08.9: 11.71 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:15:12.52 -26:30:08.9: 11.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.02
Forced photometry filter KEPT candidate at 00:15:12.52 -26:30:08.9: ref_mag=11.73 +/- 0.02 new_mean_mag=10.5594 delta=1.17 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:14:12.57 -26:36:54.3: 11.59 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:14:12.57 -26:36:54.3: 11.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.02
Forced photometry filter KEPT candidate at 00:14:12.57 -26:36:54.3: ref_mag=11.56 +/- 0.02 new_mean_mag=10.5264 delta=1.03 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 23:53:29.41 -21:31:08.1: 11.57 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 23:53:29.41 -21:31:08.1: 11.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.02
Forced photometry filter KEPT candidate at 23:53:29.41 -21:31:08.1: ref_mag=11.59 +/- 0.02 new_mean_mag=10.4454 delta=1.15 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:16:43.69 -26:51:39.5: 11.51 +/- 0.03 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:16:43.69 -26:51:39.5: 11.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.02
Forced photometry filter KEPT candidate at 00:16:43.69 -26:51:39.5: ref_mag=11.48 +/- 0.02 new_mean_mag=10.3997 delta=1.08 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:15:54.86 -26:18:04.4: 11.28 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:15:54.86 -26:18:04.4: 11.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Forced photometry filter KEPT candidate at 00:15:54.86 -26:18:04.4: ref_mag=11.29 +/- 0.01 new_mean_mag=10.2446 delta=1.05 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:21:44.29 -27:58:58.5: 11.21 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:21:44.29 -27:58:58.5: 11.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter KEPT candidate at 00:21:44.29 -27:58:58.5: ref_mag=11.20 +/- 0.01 new_mean_mag=10.2297 delta=0.97 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:31:28.69 -28:33:41.6: 11.18 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:31:28.69 -28:33:41.6: 11.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.02
Forced photometry filter KEPT candidate at 00:31:28.69 -28:33:41.6: ref_mag=11.19 +/- 0.02 new_mean_mag=10.1950 delta=1.00 (need > 0.90)
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-25-19_20.00sec_5.00C_LIGHT_0418.fits at 00:27:04.31 -28:13:05.5: 11.12 +/- 0.02 detection
Forced photometry on wcs_Scl-01-Q1b1x1_2026-07-07_04-26-13_20.00sec_5.00C_LIGHT_0419.fits at 00:27:04.31 -28:13:05.5: 11.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Forced photometry filter KEPT candidate at 00:27:04.31 -28:13:05.5: ref_mag=11.12 +/- 0.01 new_mean_mag=10.1376 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out02508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10737.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 1022s
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: 10s
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Considering the candidate 20968_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
The candidate 20968_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 04686_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04686_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 02898_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 02898_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 04580_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04580_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 03522_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 03522_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 04213_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04213_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 04852_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04852_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 03797_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 03797_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 03362_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 03362_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 03992_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 03992_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 04708_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04708_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 04862_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04862_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 02825_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 02825_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 05531_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 05531_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 10737_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 10737_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 05170_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 05170_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 05043_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 05043_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 07970_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 07970_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 04724_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 04724_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 05409_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 05409_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 03342_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 03342_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 02508_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 02508_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
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Considering the candidate 02987_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
Preparing report for the candidate 02987_fd_Scl-01-Q1b1x1_2026-08-22_03-52-03_20.00sec_0.00C_LIGHTs_0093
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 1033s
Prepared the HTML report for the field Scl-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:31:28.69 -28:33:41.6
00:26:15.63 -28:22:58.5
00:28:01.07 -28:16:52.5
00:27:04.31 -28:13:05.5
00:21:44.29 -27:58:58.5
00:22:58.55 -27:57:26.1
00:23:11.61 -27:47:41.2
00:18:28.74 -27:35:38.8
00:18:36.88 -27:25:11.5
00:21:01.91 -27:12:39.3
00:13:23.62 -26:59:02.7
00:16:37.95 -26:52:53.7
00:17:53.54 -26:51:57.0
00:16:43.69 -26:51:39.5
00:12:22.67 -26:48:02.7
00:17:20.00 -26:45:11.9
00:14:12.57 -26:36:54.3
00:15:12.52 -26:30:08.9
00:15:54.86 -26:18:04.4
00:13:55.53 -26:13:34.4
23:53:29.41 -21:31:08.1
23:56:53.77 -23:17:24.2
########### Completed Scl-01-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 ####
00:16:37.95 -26:52:53.7
00:28:01.07 -28:16:52.5
00:13:23.62 -26:59:02.7
00:23:11.61 -27:47:41.2
00:21:01.91 -27:12:39.3
00:12:22.67 -26:48:02.7
00:18:28.74 -27:35:38.8
00:22:58.55 -27:57:26.1
00:18:36.88 -27:25:11.5
00:17:53.54 -26:51:57.0
00:17:20.00 -26:45:11.9
00:26:15.63 -28:22:58.5
00:13:55.53 -26:13:34.4
23:56:53.77 -23:17:24.2
00:15:12.52 -26:30:08.9
00:14:12.57 -26:36:54.3
23:53:29.41 -21:31:08.1
00:16:43.69 -26:51:39.5
00:15:54.86 -26:18:04.4
00:21:44.29 -27:58:58.5
00:31:28.69 -28:33:41.6
00:27:04.31 -28:13:05.5
###################################################################################
00:16:37.95 -26:52:53.7 -- not an asteroid (will add it to exclusion list)
00:28:01.07 -28:16:52.5 -- not an asteroid (will add it to exclusion list)
00:13:23.62 -26:59:02.7 -- not an asteroid (will add it to exclusion list)
00:23:11.61 -27:47:41.2 -- asteroid (will NOT add it to exclusion list)
00:21:01.91 -27:12:39.3 -- not an asteroid (will add it to exclusion list)
00:12:22.67 -26:48:02.7 -- not an asteroid (will add it to exclusion list)
00:18:28.74 -27:35:38.8 -- not an asteroid (will add it to exclusion list)
00:22:58.55 -27:57:26.1 -- not an asteroid (will add it to exclusion list)
00:18:36.88 -27:25:11.5 -- not an asteroid (will add it to exclusion list)
00:17:53.54 -26:51:57.0 -- not an asteroid (will add it to exclusion list)
00:17:20.00 -26:45:11.9 -- not an asteroid (will add it to exclusion list)
00:26:15.63 -28:22:58.5 -- not an asteroid (will add it to exclusion list)
00:13:55.53 -26:13:34.4 -- not an asteroid (will add it to exclusion list)
23:56:53.77 -23:17:24.2 -- not an asteroid (will add it to exclusion list)
00:15:12.52 -26:30:08.9 -- not an asteroid (will add it to exclusion list)
00:14:12.57 -26:36:54.3 -- not an asteroid (will add it to exclusion list)
23:53:29.41 -21:31:08.1 -- not an asteroid (will add it to exclusion list)
00:16:43.69 -26:51:39.5 -- not an asteroid (will add it to exclusion list)
00:15:54.86 -26:18:04.4 -- not an asteroid (will add it to exclusion list)
00:21:44.29 -27:58:58.5 -- not an asteroid (will add it to exclusion list)
00:31:28.69 -28:33:41.6 -- not an asteroid (will add it to exclusion list)
00:27:04.31 -28:13:05.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:12:22.67 -26:48:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:23.62 -26:59:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:55.53 -26:13:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:12.57 -26:36:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:12.52 -26:30:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:54.86 -26:18:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:37.95 -26:52:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:43.69 -26:51:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:20.00 -26:45:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:53.54 -26:51:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:28.74 -27:35:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:36.88 -27:25:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:01.91 -27:12:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:44.29 -27:58:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:58.55 -27:57:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:15.63 -28:22:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:04.31 -28:13:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:01.07 -28:16:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:28.69 -28:33:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:29.41 -21:31:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:53.77 -23:17:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:12:22.67 -26:48:02.7 -- not a known variable star
00:13:23.62 -26:59:02.7 -- not a known variable star
00:13:55.53 -26:13:34.4 -- not a known variable star
00:14:12.57 -26:36:54.3 -- not a known variable star
00:15:12.52 -26:30:08.9 -- not a known variable star
00:15:54.86 -26:18:04.4 -- not a known variable star
00:16:37.95 -26:52:53.7 -- not a known variable star
00:16:43.69 -26:51:39.5 -- not a known variable star
00:17:20.00 -26:45:11.9 -- not a known variable star
00:17:53.54 -26:51:57.0 -- not a known variable star
00:18:28.74 -27:35:38.8 -- not a known variable star
00:18:36.88 -27:25:11.5 -- not a known variable star
00:21:01.91 -27:12:39.3 -- not a known variable star
00:21:44.29 -27:58:58.5 -- not a known variable star
00:22:58.55 -27:57:26.1 -- not a known variable star
00:26:15.63 -28:22:58.5 -- not a known variable star
00:27:04.31 -28:13:05.5 -- not a known variable star
00:28:01.07 -28:16:52.5 -- not a known variable star
00:31:28.69 -28:33:41.6 -- a known variable star
23:53:29.41 -21:31:08.1 -- not a known variable star
23:56:53.77 -23:17:24.2 -- a known variable star
Found 19 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
21 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
00:12:22.67 -26:48:02.7
00:13:23.62 -26:59:02.7
00:13:55.53 -26:13:34.4
00:14:12.57 -26:36:54.3
00:15:12.52 -26:30:08.9
00:15:54.86 -26:18:04.4
00:16:37.95 -26:52:53.7
00:16:43.69 -26:51:39.5
00:17:20.00 -26:45:11.9
00:17:53.54 -26:51:57.0
00:18:28.74 -27:35:38.8
00:18:36.88 -27:25:11.5
00:21:01.91 -27:12:39.3
00:21:44.29 -27:58:58.5
00:22:58.55 -27:57:26.1
00:26:15.63 -28:22:58.5
00:27:04.31 -28:13:05.5
00:28:01.07 -28:16:52.5
00:31:28.69 -28:33:41.6
23:53:29.41 -21:31:08.1
23:56:53.77 -23:17:24.2
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461274.86888543 -observatory V36
09:45:19.10 +15:18:26.6 Mercury (-1.7mag)
12:50:14.99 -07:46:57.9 Venus (-4.5mag)
06:29:54.33 +23:38:58.6 Mars (1.3mag)
08:55:30.67 +17:53:01.4 Jupiter (-1.8mag)
00:54:49.12 +03:01:31.4 Saturn (0.5mag)
04:13:02.31 +21:00:19.4 Uranus (5.7mag)
00:15:07.95 +00:06:16.1 Neptune (7.7mag)
20:26:50.55 -23:35:12.3 Pluto (14.5mag)
17:27:44.53 -28:28:53.8 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 Aug 22 03:58 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461274.86888543:
08:55:34.07 +17:52:45.7 Io (6.1mag)
08:55:38.24 +17:52:27.2 Europa (6.3mag)
08:55:46.85 +17:51:47.7 Ganymede (5.6mag)
08:55:11.37 +17:54:32.1 Callisto (6.9mag)
08:52:58.90 +18:01:02.2 Himalia (15.7mag)
08:55:29.41 +17:53:08.0 Thebe (16.6mag)
08:52:38.14 +17:56:54.3 Elara (17.7mag)
08:59:38.26 +17:26:16.3 Pasiphae (17.9mag)
08:57:43.74 +18:06:36.6 Carme (19.0mag)
00:54:45.44 +03:01:56.8 Titan (8.4mag)
00:54:53.73 +03:01:22.6 Rhea (9.7mag)
00:55:24.57 +03:03:12.4 Iapetus (11.1mag)
00:54:56.91 +03:01:48.3 Hyperion (14.4mag)
00:53:53.87 +02:52:56.7 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 22 03:58 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461274.86888543:
20:11:55.88 -14:03:00.1 JWST
17:35:17.96 +34:58:35.1 Chandra
11:13:00.16 -60:00:25.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 22 03:58 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461274.86888543 -observatory V36
03:28:15.98 +18:26:31.6 17.5mag P/1996 R2 (Lagerkvist)
17:59:54.62 -34:28:34.4 14.2mag P/2010 H2 (Vales)
07:06:30.96 -69:29:27.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:08.77 +33:18:28.2 17.7mag C/2017 K2 (PANSTARRS)
04:21:08.58 +42:24:40.9 17.5mag P/2021 N1 (ZTF)
22:26:43.25 +30:22:36.1 17.4mag C/2022 E2 (ATLAS)
06:56:55.37 +26:16:59.8 16.8mag C/2022 N2 (PANSTARRS)
10:34:43.15 +27:51:05.5 17.0mag C/2022 QE78 (ATLAS)
09:38:18.68 +05:17:59.4 18.0mag C/2022 R6 (PANSTARRS)
15:15:40.11 -12:52:43.6 18.0mag P/2023 B1 (PANSTARRS)
20:53:25.19 +64:04:08.6 18.0mag C/2023 H5 (Lemmon)
15:36:28.46 -14:14:03.0 14.6mag C/2023 R1 (PANSTARRS)
08:23:16.33 +32:00:47.5 15.5mag C/2024 E1 (Wierzchos)
15:05:42.21 +15:30:15.8 17.8mag C/2024 G6 (ATLAS)
18:46:50.65 +43:29:22.9 13.7mag C/2024 J3 (ATLAS)
20:49:23.50 +49:41:19.0 17.5mag C/2024 R4 (PANSTARRS)
05:25:46.22 -12:53:57.6 15.3mag C/2024 T5 (ATLAS)
07:04:37.05 +21:36:18.7 17.9mag C/2025 J1 (Borisov)
10:53:17.18 +19:57:25.4 17.1mag C/2025 V2 (Rankin)
13:07:24.22 +01:21:12.2 16.9mag C/2025 Y1 (ATLAS)
16:10:30.49 +76:17:17.8 16.5mag C/2026 A2 (Bok)
03:09:55.55 +46:20:59.3 17.3mag C/2026 B2 (Sun-Gao)
11:58:51.85 +09:55:44.4 17.4mag A/2026 E1
22:12:24.91 -32:18:20.5 7.1mag 10P/Tempel
11:37:43.73 -04:19:17.0 16.3mag 29P/Schwassmann-Wachmann
11:36:26.10 +00:01:13.3 17.4mag 63P/Wild
00:51:37.32 -06:06:11.8 15.4mag 65P/Gunn
06:06:48.35 +20:14:32.9 13.7mag 78P/Gehrels
20:25:49.33 -25:00:02.0 17.5mag 84P/Giclas
03:12:00.16 +14:32:15.8 16.9mag 88P/Howell
08:30:31.91 +25:35:04.8 16.4mag 93P/Lovas
04:47:36.17 +22:25:02.7 17.2mag 112P/Urata-Niijima
06:42:35.97 +28:17:45.1 16.1mag 114P/Wiseman-Skiff
09:51:40.58 +24:05:31.5 14.9mag 123P/West-Hartley
12:12:32.55 -15:36:33.7 17.3mag 124P/Mrkos
05:56:46.04 +21:01:44.9 16.0mag 128P/Shoemaker-Holt
06:51:58.09 +18:06:00.7 17.9mag 131P/Mueller
23:59:37.28 +03:06:00.6 17.4mag 139P/Vaisala-Oterma
03:09:36.64 -18:37:33.9 12.8mag 161P/Hartley-IRAS
08:03:38.99 +38:07:18.4 16.1mag 162P/Siding Spring
11:04:04.68 +29:55:02.1 12.2mag 169P/NEAT
03:06:11.70 +09:23:39.0 17.6mag 220P/McNaught
20:16:20.50 -51:48:30.8 18.0mag 259P/Garradd
04:03:18.04 +30:49:59.9 15.3mag 260P/McNaught
07:47:20.13 +37:05:15.2 17.3mag 295P/LINEAR
15:16:11.54 +01:33:12.9 17.8mag 391P/Kowalski
09:13:43.50 +17:40:02.2 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 22 03:58 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
-rw-r--r-- 1 apache apache 5.7K Aug 22 03:58 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 22 03:58 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:44:08.771 +29:07:45.05 AT 2026xfr 2026-01-14.38 20.4
23:28:59.311 -21:41:17.71 AT 2026xfq 2026-07-19.57 21.15
20:34:55.430 -31:12:10.98 AT 2026xfp 2026-07-14.44 20
13:01:30.092 +38:12:35.50 AT 2026xfo 2026-06-23.28 20.85
23:22:05.758 +18:57:29.94 AT 2026xfn 2026-07-25.52 21.28
10:13:35.246 -20:37:42.73 AT 2026xfm 2026-01-27.58 21
21:57:25.287 +03:48:20.98 AT 2026xfl 2026-07-16.55 21.68
14:26:07.382 +33:39:52.18 AT 2026xfk 2026-06-13.34 20.9
02:09:31.559 -03:10:04.80 AT 2026xfj 2026-01-17.24 21.98
20:17:01.562 -20:06:27.94 AT 2026xfi 2026-05-20.56 20.93
21:08:09.912 -21:12:24.85 AT 2026xfh 2026-06-19.58 20.9
20:08:20.135 -25:53:36.34 AT 2026xfg 2026-07-19.45 20.74
14:51:25.078 +41:07:07.07 AT 2026xff 2026-06-13.34 21.62
22:33:15.210 +12:04:33.49 AT 2026xfe 2026-06-21.53 20.23
13:52:05.795 +29:21:47.19 AT 2026xfd 2026-04-24.32 20.92
13:30:27.613 +10:38:39.93 AT 2026xfc 2026-04-20.32 21.07
13:40:18.442 +39:30:10.71 AT 2026xfb 2026-05-24.29 20.6
20:02:32.611 -29:31:03.47 AT 2026xfa 2026-06-16.52 19.85
21:35:00.881 +03:50:25.49 AT 2026xez 2026-07-16.55 21.5
08:33:56.550 +06:59:43.01 AT 2026xey 2026-01-24.36 22.17
-rw-r--r-- 1 apache apache 87K Aug 22 03:58 tns_transients_list.txt
