This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.03 15:53:22.81 +48:03:08.3
76.17213 49.13280 galactic Her Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:53:22.81 +48:03:08.3 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.032 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:22.81 +48:03:08.3: 13.22 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:22.81 +48:03:08.3: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 53 22.81 +48 03 08.3 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.63 15:57:21.97 +47:41:19.0
75.39866 48.56706 galactic Her Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1399607521098425216 | 15:57:21.93 +47:41:18.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.558+/-0.028 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:57:21.97 +47:41:19.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:57:21.97 +47:41:19.0: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 57 21.97 +47 41 19.0 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1399607521098425216,2461237.8581,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1399607521098425216 20260716.3581 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.28 15:47:14.71 +48:13:37.7
76.83925 50.07683 galactic Boo Second-epoch detections are separated by 1.3" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1401410312147206016
Type: ROT
# Max. Min./Amp. JD0 Period
13.290 G 13.330 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:47:14.71 +48:13:37.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:47:14.71 +48:13:37.7: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 1401410312147206016,2461237.8581,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1401410312147206016 20260716.3581 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 10.88 15:53:40.38 +48:13:32.5
76.41061 49.04304 galactic Her Second-epoch detections are separated by 0.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J238.4301+48.2178 | 15:53:43.22 +48:13:04.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.028 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:40.38 +48:13:32.5: 11.80 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:40.38 +48:13:32.5: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 53 40.38 +48 13 32.5 10.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.4301+48.2178,2461237.8581,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J238.4301+48.2178 20260716.3581 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.89 15:37:54.34 +49:51:39.8
80.02537 51.03314 galactic Boo Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1402656161900174208 | 15:37:54.34 +49:51:39.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.478+/-0.032 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:37:54.34 +49:51:39.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:37:54.34 +49:51:39.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1402656161900174208,2461237.8581,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1402656161900174208 20260716.3581 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.75 15:58:58.19 +47:13:43.3
74.63345 48.40048 galactic Her Second-epoch detections are separated by 2.4" and 6.4 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 | 15:58:58.19 +47:13:43.3 (user input) | T | P | (position from user input) J-Ks=0.287+/-0.033 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:58:58.19 +47:13:43.3: 12.80 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:58:58.19 +47:13:43.3: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 58 58.19 +47 13 43.3 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.63 15:35:13.78 +42:18:51.2
68.33624 53.51800 galactic Boo Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:35:13.78 +42:18:51.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.388+/-0.028 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:35:13.78 +42:18:51.2: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:35:13.78 +42:18:51.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8581,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.43 15:51:30.04 +47:55:26.3
76.09996 49.46919 galactic Her Second-epoch detections are separated by 1.6" and 6.9 pix
The object was found in VSX 1" NSVS 5204213
Type: EA
# Max. Min./Amp. JD0 Period
12.950 R1 Y 0.550 R1 1.319018090000
The object was not found in astcheck.
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:30.04 +47:55:26.3: 12.75 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:30.04 +47:55:26.3: 12.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 51 30.04 +47 55 26.3 11.4 U Her 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
NSVS 5204213,2461237.8581,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5204213 20260716.3581 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.86 15:51:36.21 +42:03:25.8
67.12448 50.56683 galactic Her Second-epoch detections are separated by 1.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:51:36.21 +42:03:25.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.528+/-0.027 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:36.21 +42:03:25.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:36.21 +42:03:25.8: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 51 36.21 +42 03 25.8 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.17 15:53:18.41 +48:26:55.8
76.76343 49.04656 galactic Her Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:53:18.41 +48:26:55.8 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.392+/-0.033 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:18.41 +48:26:55.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:18.41 +48:26:55.8: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 53 18.41 +48 26 55.8 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.16 15:51:17.54 +47:50:55.7
76.00119 49.52167 galactic Her Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J237.8231+47.8485 | 15:51:17.54 +47:50:55.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.338+/-0.034 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:17.54 +47:50:55.7: 13.37 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:17.54 +47:50:55.7: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 51 17.54 +47 50 55.7 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.8231+47.8485,2461237.8581,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J237.8231+47.8485 20260716.3581 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.10 16:01:27.09 +47:46:21.4
75.30123 47.87803 galactic Her Second-epoch detections are separated by 1.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:01:27.09 +47:46:21.4 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.032 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 16:01:27.09 +47:46:21.4: 13.38 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 16:01:27.09 +47:46:21.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 16 01 27.09 +47 46 21.4 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.47 15:34:46.93 +42:12:59.1
68.20167 53.61817 galactic Boo Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1391061773129359360 | 15:34:46.85 +42:12:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.029 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:46.93 +42:12:59.1: 12.41 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:46.93 +42:12:59.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1391061773129359360,2461237.8581,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1391061773129359360 20260716.3581 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.04 15:34:38.14 +42:16:01.8
68.29450 53.63491 galactic Boo Second-epoch detections are separated by 2.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:34:38.14 +42:16:01.8 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.030 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:38.14 +42:16:01.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:38.14 +42:16:01.8: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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,2461237.8581,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 12.17 15:47:17.82 +48:06:04.0
76.64647 50.10253 galactic Boo Second-epoch detections are separated by 2.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:47:17.82 +48:06:04.0 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.488+/-0.028 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:47:17.82 +48:06:04.0: 13.53 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:47:17.82 +48:06:04.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 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
target,2461237.8581,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.88 15:50:00.41 +48:35:36.4
77.19472 49.53685 galactic Her Second-epoch detections are separated by 1.8" and 6.3 pix
The object was found in VSX 1" Gaia DR3 1401441613868818176
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.860 G 12.900 G F
The object was not found in astcheck.
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:50:00.41 +48:35:36.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:50:00.41 +48:35:36.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 50 00.41 +48 35 36.4 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1401441613868818176,2461237.8581,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1401441613868818176 20260716.3581 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.47 15:46:03.49 +47:55:51.4
76.47758 50.34789 galactic Boo Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1401398762978428928 | 15:46:03.39 +47:55:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:46:03.49 +47:55:51.4: 12.31 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:46:03.49 +47:55:51.4: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 1401398762978428928,2461237.8581,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1401398762978428928 20260716.3581 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.99 15:53:34.02 +48:09:18.0
76.31262 49.07750 galactic Her Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:53:34.02 +48:09:18.0 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.032 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:34.02 +48:09:18.0: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:34.02 +48:09:18.0: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 53 34.02 +48 09 18.0 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.81 15:59:21.51 +47:08:04.2
74.47430 48.35510 galactic Her Second-epoch detections are separated by 1.1" and 6.6 pix
The object was found in VSX12" Gaia DR3 1398785949689793920
Type: ROT
# Max. Min./Amp. JD0 Period
13.950 G 13.980 G K
The object was not found in astcheck.
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:59:21.51 +47:08:04.2: 12.69 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:59:21.51 +47:08:04.2: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 59 21.51 +47 08 04.2 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1398785949689793920,2461237.8581,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1398785949689793920 20260716.3581 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.21 15:50:50.97 +48:09:37.0
76.49424 49.51498 galactic Her Second-epoch detections are separated by 0.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1401370862870866688 | 15:50:50.98 +48:09:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.026 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:50:50.97 +48:09:37.0: 12.31 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:50:50.97 +48:09:37.0: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 50 50.97 +48 09 37.0 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1401370862870866688,2461237.8581,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1401370862870866688 20260716.3581 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.56 15:53:31.06 +48:11:32.6
76.37104 49.07631 galactic Her Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:53:31.06 +48:11:32.6 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.030 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:31.06 +48:11:32.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:31.06 +48:11:32.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 53 31.06 +48 11 32.6 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 10.46 15:34:58.41 +42:20:30.4
68.39724 53.55907 galactic Boo Second-epoch detections are separated by 0.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1391065797515298048 | 15:34:58.48 +42:20:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.690+/-0.028 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:58.41 +42:20:30.4: 11.50 +/- 0.00 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:58.41 +42:20:30.4: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1391065797515298048,2461237.8581,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1391065797515298048 20260716.3581 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.74 16:00:14.27 +46:04:07.3
72.85563 48.41064 galactic Her Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1398468809304947840 | 16:00:14.34 +46:04:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.399+/-0.035 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 16:00:14.27 +46:04:07.3: 12.60 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 16:00:14.27 +46:04:07.3: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 16 00 14.27 +46 04 07.3 11.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1398468809304947840,2461237.8581,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1398468809304947840 20260716.3581 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.16 15:53:14.91 +48:13:21.0
76.43247 49.11235 galactic Her Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1399872645135246592 | 15:53:14.90 +48:13:20.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.030 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:14.91 +48:13:21.0: 12.25 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:14.91 +48:13:21.0: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 53 14.91 +48 13 21.0 11.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1399872645135246592,2461237.8581,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1399872645135246592 20260716.3581 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.63 16:01:20.77 +47:49:32.1
75.38397 47.88434 galactic Her Second-epoch detections are separated by 2.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1399650200189063168 | 16:01:20.87 +47:49:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.657+/-0.032 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 16:01:20.77 +47:49:32.1: 12.59 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 16:01:20.77 +47:49:32.1: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 16 01 20.77 +47 49 32.1 11.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1399650200189063168,2461237.8581,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1399650200189063168 20260716.3581 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.14 15:51:27.08 +47:41:07.5
75.74707 49.53595 galactic Her Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1398342876567506816 | 15:51:27.16 +47:41:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.493+/-0.029 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:27.08 +47:41:07.5: 12.19 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:27.08 +47:41:07.5: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 51 27.08 +47 41 07.5 11.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1398342876567506816,2461237.8581,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1398342876567506816 20260716.3581 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.18 15:46:51.41 +48:12:24.9
76.83632 50.14458 galactic Boo Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1401420478333068928 | 15:46:51.45 +48:12:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.242+/-0.025 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:46:51.41 +48:12:24.9: 12.15 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:46:51.41 +48:12:24.9: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1401420478333068928,2461237.8581,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1401420478333068928 20260716.3581 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 10.95 15:34:38.64 +42:17:37.6
68.33801 53.62820 galactic Boo Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J233.6606+42.2937 | 15:34:38.56 +42:17:37.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.300+/-0.028 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:38.64 +42:17:37.6: 12.11 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:38.64 +42:17:37.6: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 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
ATO J233.6606+42.2937,2461237.8581,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J233.6606+42.2937 20260716.3581 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.03 15:45:47.56 +48:24:50.6
77.22376 50.25732 galactic Boo Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1401614821309554176 | 15:45:47.62 +48:24:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.296+/-0.025 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:45:47.56 +48:24:50.6: 12.12 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:45:47.56 +48:24:50.6: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1401614821309554176,2461237.8581,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1401614821309554176 20260716.3581 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.79 15:45:43.11 +48:32:07.6
77.41130 50.23488 galactic Boo Second-epoch detections are separated by 2.0" and 6.1 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 | 15:45:43.11 +48:32:07.6 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.776+/-0.026 (K)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:45:43.11 +48:32:07.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:45:43.11 +48:32:07.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461237.8581,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.01 15:59:20.93 +47:14:04.7
74.62231 48.33629 galactic Her Second-epoch detections are separated by 0.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1398787629021725952 | 15:59:20.90 +47:14:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:59:20.93 +47:14:04.7: 11.97 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:59:20.93 +47:14:04.7: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 59 20.93 +47 14 04.7 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1398787629021725952,2461237.8581,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1398787629021725952 20260716.3581 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.88 15:50:56.32 +48:08:36.8
76.46349 49.50486 galactic Her Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:50:56.32 +48:08:36.8 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.257+/-0.028 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:50:56.32 +48:08:36.8: 13.20 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:50:56.32 +48:08:36.8: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 50 56.32 +48 08 36.8 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 16.3581 2461237.8581 11.65 15:44:15.57 +48:12:45.8
77.03343 50.55866 galactic Boo Second-epoch detections are separated by 1.2" and 6.4 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 | Large-amplitude variable Gaia DR2 1401514971909690880 | 15:44:15.57 +48:12:45.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G2 (LAMOST DR5) J-Ks=0.289+/-0.027 (F)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:44:15.57 +48:12:45.8: 12.90 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:44:15.57 +48:12:45.8: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1401514971909690880,2461237.8581,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1401514971909690880 20260716.3581 11.65CV 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 07 16.3581 2461237.8581 11.95 15:51:16.93 +47:37:53.0
75.67700 49.57675 galactic Her Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:51:16.93 +47:37:53.0 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.030 (G)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:16.93 +47:37:53.0: 13.17 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:16.93 +47:37:53.0: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 16.3581* 15 51 16.93 +47 37 53.0 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461237.8581,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260716.3581 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461199.78284559 08.06.2026 06:47:07.859 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
First image: 2461199.78284559 08.06.2026 06:47:07.859 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Last image: 2461237.85835877 16.07.2026 08:35:52.198 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5861
Objects passed selection criteria: 5826
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 3301.5
Average stars matched: 3221 (97.5617 %)
Memory usage VmPeak: 115608 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 03:51:57 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461199.78284559 08.06.2026 06:47:07.859 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
First image: 2461199.78284559 08.06.2026 06:47:07.859 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Last image: 2461237.85835877 16.07.2026 08:35:52.198 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 48
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.06
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: 10 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 32321
Objects passed selection criteria: 32208
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: 19518.8
Average stars matched: 18816.2 (96.4009 %)
Memory usage VmPeak: 140788 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 15 19:22:19 CDT 2026
VaST build number 1.0rc89-155-g87a29d73
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 16 03:54:17 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
SExtractor catalog cache: saved Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.cat to cache
SExtractor catalog cache: saved Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.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/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.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: 2461237.85786345
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_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits exists and is non-empty
Saving wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits to local_wcs_cache/
'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits' -> 'local_wcs_cache/wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits'
wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits exists and is non-empty
Saving wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits to local_wcs_cache/
'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits' -> 'local_wcs_cache/wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits'
wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits exists and is non-empty
Saving wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits to local_wcs_cache/
'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits' -> 'local_wcs_cache/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits'
wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits exists and is non-empty
Saving wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits to local_wcs_cache/
'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits' -> 'local_wcs_cache/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits (1st reference image)
verification OK: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:36:01.806 +45:59:16.16 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/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_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits (1st new image)
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:35:59.158 +45:59:40.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:36:01.806 +45:59:16.16
Second-epoch image center 15:35:59.158 +45:59:40.46
Angular distance between the image centers 0.0102 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits (2nd new image)
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:35:55.898 +45:59:21.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:36:01.806 +45:59:16.16
Second-epoch image center 15:35:55.898 +45:59:21.29
Angular distance between the image centers 0.0172 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 15:35:59.158 +45:59:40.46
Second-epoch second image center 15:35:55.898 +45:59:21.29
Angular distance between the image centers 0.01084 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/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits &> /tmp/tmp.B8JX0fQm9Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits &> /tmp/tmp.yLQhQz0Pon
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits &> /tmp/tmp.4IppPWMJHJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits &> /tmp/tmp.WVZyhgKOX1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.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_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits and wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.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_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits and wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
Found non-empty wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits and wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
The reference image (wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits) and catalog (wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat) found
'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat' -> 'wcsmag.cat'
Read 7921 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.8223 to 246.3489 deg, Dec +40.2987 to +51.2488 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 221.8223 to 246.3489 deg, Dec 40.2987 to 51.2488 deg
Loaded 5355 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): 4009 out of 4124 total matches.
Matched with Tycho-2 4124 out of 7921 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.737400
a=0.000000 b=1.000000 c=22.737400
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7921 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.8223 to 246.3489 deg, Dec +40.2987 to +51.2488 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 221.8223 to 246.3489 deg, Dec 40.2987 to 51.2488 deg
Loaded 5355 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): 4009 out of 4124 total matches.
Matched with Tycho-2 4124 out of 7921 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits:
Forced-photometry filter: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits -> calib.txt_param_ref_wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits (aperture=6.3)
Read 7913 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.8224 to 246.3488 deg, Dec +40.2707 to +51.2503 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 221.8224 to 246.3488 deg, Dec 40.2707 to 51.2503 deg
Loaded 5369 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): 4018 out of 4127 total matches.
Matched with Tycho-2 4127 out of 7913 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits:
Forced-photometry filter: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits -> calib.txt_param_ref_wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
2.3 pix Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
2.2 pix fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
2.3 pix fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
2.3 pix wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
2.3 pix wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Limiting magnitude estimates:
15.4 mag. Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
15.4 mag. Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
12.2 mag. fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
12.7 mag. fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 9.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.B8JX0fQm9Y (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits' -> 'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Checking if the catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
WCS catalog name: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, bad_region=1731, passed=7921
Got 7921 stars (including 5855 good ones) from the SExtractor catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
util/solve_plate_with_UCAC5 got 7921 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits N_match=982 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.391 n_q1=325 n_q2=192 n_q3=283 n_q4=182 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits -region wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.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.yLQhQz0Pon (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits' -> 'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
WCS-calibrated image found: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Checking if the catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
WCS catalog name: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=398, bad_region=1710, passed=7913
Got 7913 stars (including 5870 good ones) from the SExtractor catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat
util/solve_plate_with_UCAC5 got 7913 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits N_match=982 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.335 n_q1=321 n_q2=190 n_q3=284 n_q4=187 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits -region wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.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.4IppPWMJHJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Checking if the catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
WCS catalog name: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=18, bad_region=23, passed=434
Got 434 stars (including 394 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat
util/solve_plate_with_UCAC5 got 434 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 652 to 707 (Dec 40.6 to 51.0)
Done reading UCAC5 zone files...
Matched 377 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 377 matched stars entering correct_measured_positions(), 317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 377 matched stars entering correct_measured_positions(), 340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 652 to 707 (Dec 40.6 to 51.0)
Done reading UCAC5 zone files...
Matched 376 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 376 stars left (next iteration limit 414)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits N_match=376 sigma_overall_arcsec=0.559 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.720 sigma_q3_arcsec=0.619 sigma_q4_arcsec=0.550 n_q1=160 n_q2=39 n_q3=157 n_q4=20 worst_quadrant_to_overall_ratio=1.289
The image catalog is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits -region wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.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.WVZyhgKOX1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Checking if the catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS catalog name: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=18, bad_region=21, passed=479
Got 479 stars (including 441 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 652 to 706 (Dec 40.5 to 51.0)
Done reading UCAC5 zone files...
Matched 420 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 420 matched stars entering correct_measured_positions(), 376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 420 matched stars entering correct_measured_positions(), 404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 652 to 706 (Dec 40.5 to 51.0)
Done reading UCAC5 zone files...
Matched 420 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 420 matched stars entering correct_measured_positions(), 409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 420 matched stars entering correct_measured_positions(), 409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 420 stars left (next iteration limit 462)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits N_match=420 sigma_overall_arcsec=0.749 sigma_q1_arcsec=0.712 sigma_q2_arcsec=0.773 sigma_q3_arcsec=0.767 sigma_q4_arcsec=0.657 n_q1=156 n_q2=31 n_q3=215 n_q4=18 worst_quadrant_to_overall_ratio=1.032
The image catalog is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits -region wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits sigma_overall=0.360 worst_q_ratio=1.171
ref2=Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits sigma_overall=0.352 worst_q_ratio=1.196
new1=fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits sigma_overall=0.559 worst_q_ratio=1.289
new2=fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits sigma_overall=0.749 worst_q_ratio=1.032
reference average sigma_overall=0.356 worst_q_ratio=1.1835
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 2nd new image (fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits) flagged: sigma=0.749 (ref avg 0.356), ratio=1.032 (ref avg 1.1835), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/lib/make_outxyls_for_astrometric_calibration found 472 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3835222.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3835222.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
log-odds ratio 38.306 (4.32601e+16), 7 match, 0 conflict, 9 distractors, 46 index.
RA,Dec = (233.987,45.9828), pixel scale 5.94307 arcsec/pix.
Hit/miss: Hit/miss: +--++-+--+--+--+(best)-----------------+------+-----------+-----------------------------------------------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out3835222.solved to indicate this.
Field: out3835222.xyls
Field center: (RA,Dec) = (233.984789, 45.990250) deg.
Field center: (RA H:M:S, Dec D:M:S) = (15:35:56.349, +45:59:24.901).
Field size: 15.7369 x 10.5309 degrees
Field rotation angle: up is 179.365 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits' -> 'fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 16 03:53 fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
-rw-r--r-- 1 apache apache 12K Jul 16 03:53 out3835222.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits for reading... done!
Creating new image file (wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits (fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3835222.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3835222.axy"...
Only searching for solutions within 15.6583 degrees of RA,Dec (233.984,45.9894)
log-odds ratio 87.3102 (8.28628e+37), 11 match, 0 conflict, 5 distractors, 21 index.
RA,Dec = (233.986,45.9944), pixel scale 5.95464 arcsec/pix.
Hit/miss: Hit/miss: +-+++-+-+--+++++(best)-------------------------+---+------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3835222.solved to indicate this.
Field: out3835222.xyls
Field center: (RA,Dec) = (233.983707, 45.991742) deg.
Field center: (RA H:M:S, Dec D:M:S) = (15:35:56.090, +45:59:30.271).
Field size: 15.7383 x 10.533 degrees
Field rotation angle: up is 179.366 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 16 03:53 fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
-rw-r--r-- 1 apache apache 12K Jul 16 03:53 out3835222.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits for reading... done!
Creating new image file (wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 3304 sources.
Solving...
Reading file "./wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.axy"...
Verifying WCS using indices with quads of size [63.3841, 950.166] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
log-odds ratio 102.948 (5.12716e+44), 11 match, 0 conflict, 102 distractors, 12 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: -+-+-----+++--------++---+---+-------+--------------------------------------------------------------
--> log-odds 102.948
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 162.792 (5.00639e+70), 17 match, 0 conflict, 96 distractors, 21 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++--+--+++------+-++---+---+-------+--------------------------------+-------------+---------------
--> log-odds 162.792
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 277.555 (3.47324e+120), 31 match, 0 conflict, 82 distractors, 46 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++--+-++++-+---+++++---+---++-+-+--+----+----------+---+------------+-----+-------+-------+-------
--> log-odds 277.555
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 439.99 (1.2173e+191), 63 match, 0 conflict, 288 distractors, 94 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-++++-++-+-+-----+-+-++---+-+-------+-++-----+-------+------++-------
--> log-odds 439.99
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 963.916 (inf), 150 match, 0 conflict, 734 distractors, 192 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-+-----++++++---+++----+--+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 963.916
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 1656.1 (inf), 270 match, 0 conflict, 983 distractors, 371 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-++----++++++---+++++--++-+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 1656.1
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 2892.78 (inf), 489 match, 0 conflict, 1051 distractors, 726 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-++-+--++++++---+++++--++-+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 2892.78
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 4958.82 (inf), 911 match, 0 conflict, 1604 distractors, 1447 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-++-+--++++++---+++++--++-+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 4958.82
Verifying WCS using indices with quads of size [63.3841, 950.166] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
log-odds ratio 102.948 (5.12716e+44), 11 match, 0 conflict, 102 distractors, 12 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: -+-+-----+++--------++---+---+-------+--------------------------------------------------------------
--> log-odds 102.948
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 162.792 (5.00639e+70), 17 match, 0 conflict, 96 distractors, 21 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++--+--+++------+-++---+---+-------+--------------------------------+-------------+---------------
--> log-odds 162.792
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 277.555 (3.47324e+120), 31 match, 0 conflict, 82 distractors, 46 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++--+-++++-+---+++++---+---++-+-+--+----+----------+---+------------+-----+-------+-------+-------
--> log-odds 277.555
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 439.99 (1.2173e+191), 63 match, 0 conflict, 288 distractors, 94 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-++++-++-+-+-----+-+-++---+-+-------+-++-----+-------+------++-------
--> log-odds 439.99
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 963.916 (inf), 150 match, 0 conflict, 734 distractors, 192 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-+-----++++++---+++----+--+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 963.916
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 1656.1 (inf), 270 match, 0 conflict, 983 distractors, 371 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-++----++++++---+++++--++-+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 1656.1
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 2892.78 (inf), 489 match, 0 conflict, 1051 distractors, 726 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-++-+--++++++---+++++--++-+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 2892.78
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 4958.82 (inf), 911 match, 0 conflict, 1604 distractors, 1447 index.
RA,Dec = (233.985,45.9926), pixel scale 5.95342 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++++++-+---++++++--+++-++-+++++++-+-++-+--++++++---+++++--++-+-++-++--++--++--++--+-+++-+-+-+-
--> log-odds 4958.82
Got 16 solutions.
Field: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Field center: (RA,Dec) = (233.987726, 45.989996) deg.
Field center: (RA H:M:S, Dec D:M:S) = (15:35:57.054, +45:59:23.984).
Field size: 15.7536 x 10.5357 degrees
Field rotation angle: up is 179.365 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.new"...
renamed 'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.new' -> 'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits'
Checking if the catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Generating wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat from image00004.cat
Catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits created.
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Image size: 941.0'x625.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:35:56.771 +45:59:20.97 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 479 stars ###
'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/correct_sextractor_wcs_catalog_usingxy2sky3852703.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS catalog name: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=18, bad_region=21, passed=479
Got 479 stars (including 441 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 652 to 706 (Dec 40.5 to 51.0)
Done reading UCAC5 zone files...
Matched 422 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 422 matched stars entering correct_measured_positions(), 377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 422 matched stars entering correct_measured_positions(), 405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 652 to 706 (Dec 40.5 to 51.0)
Done reading UCAC5 zone files...
Matched 421 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 421 matched stars entering correct_measured_positions(), 404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.06"
Accuracy estimation diagnostic: 421 matched stars entering correct_measured_positions(), 404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.04"
Excluding outliers - 421 stars left (next iteration limit 464)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits N_match=421 sigma_overall_arcsec=1.501 sigma_q1_arcsec=1.228 sigma_q2_arcsec=2.303 sigma_q3_arcsec=1.346 sigma_q4_arcsec=2.568 n_q1=157 n_q2=31 n_q3=215 n_q4=18 worst_quadrant_to_overall_ratio=1.710
The image catalog is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits -region wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits): sigma 0.749->1.501, ratio 1.032->1.710; reverting to order 3
WARNING: 2nd new image has sigma_overall_arcsec=1.501 -- 4.22x the reference average (0.356); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217_astrometric_residuals.png (982 matched stars from wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218_astrometric_residuals.png (982 matched stars from wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238_astrometric_residuals.png (376 matched stars from wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239_astrometric_residuals.png (420 matched stars from wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.64 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits'
Saving fully-calibrated image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits'
Preparing the HTML report for the field Boo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Boo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
SExtractor catalog cache: saved Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.cat to cache
SExtractor catalog cache: saved Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Creating symlink local_wcs_cache/wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits exists and is non-empty
wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits exists and is non-empty
wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits exists and is non-empty
wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits (1st reference image)
verification OK: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:36:01.806 +45:59:16.16 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/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_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits (1st new image)
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:35:59.158 +45:59:40.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:36:01.806 +45:59:16.16
Second-epoch image center 15:35:59.158 +45:59:40.46
Angular distance between the image centers 0.0102 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits (2nd new image)
verification OK: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:35:55.898 +45:59:21.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:36:01.806 +45:59:16.16
Second-epoch image center 15:35:55.898 +45:59:21.29
Angular distance between the image centers 0.0172 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 15:35:59.158 +45:59:40.46
Second-epoch second image center 15:35:55.898 +45:59:21.29
Angular distance between the image centers 0.01084 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/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits &> /tmp/tmp.9sklhLGCa0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits &> /tmp/tmp.VlNDttc92I
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits &> /tmp/tmp.uiUABR2uhO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits &> /tmp/tmp.mi0dblkZpp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.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_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits and wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.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_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits and wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
Found non-empty wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits and wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
The reference image (wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits) and catalog (wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat) found
'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat' -> 'wcsmag.cat'
Read 41579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.7536 to 246.3959 deg, Dec +40.2501 to +51.2514 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 221.7536 to 246.3959 deg, Dec 40.2501 to 51.2514 deg
Loaded 5409 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): 3842 out of 4144 total matches.
Matched with Tycho-2 4144 out of 41579 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.618000
a=0.000000 b=1.000000 c=22.618000
From vast_summary.log: estimated ref. image limiting mag.: -7.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 41579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.7536 to 246.3959 deg, Dec +40.2501 to +51.2514 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 221.7536 to 246.3959 deg, Dec 40.2501 to 51.2514 deg
Loaded 5409 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): 3842 out of 4144 total matches.
Matched with Tycho-2 4144 out of 41579 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits:
Forced-photometry filter: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits -> calib.txt_param_ref_wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits (aperture=4.9)
Read 41392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.7512 to 246.3488 deg, Dec +40.2546 to +51.2613 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 221.7512 to 246.3488 deg, Dec 40.2546 to 51.2613 deg
Loaded 5396 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): 3842 out of 4142 total matches.
Matched with Tycho-2 4142 out of 41392 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits:
Forced-photometry filter: calibrated wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits -> calib.txt_param_ref_wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
2.2 pix Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
2.1 pix fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
2.1 pix fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
2.2 pix wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
2.2 pix wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Limiting magnitude estimates:
15.6 mag. Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
15.5 mag. Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
12.3 mag. fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
12.4 mag. fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9sklhLGCa0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits' -> 'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
Checking if the catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits
WCS catalog name: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1789, bad_region=6345, passed=41566
Got 41566 stars (including 33770 good ones) from the SExtractor catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat
util/solve_plate_with_UCAC5 got 41566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 35814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 35814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 35814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits N_match=980 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.444 sigma_q4_arcsec=0.386 n_q1=322 n_q2=191 n_q3=284 n_q4=183 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits -region wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.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.VlNDttc92I (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits' -> 'wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
WCS_IMAGE_NAME=wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
WCS-calibrated image found: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
Checking if the catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits alredy exist and is non-empty...
Catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat corresponding to the image wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits
WCS catalog name: wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1780, bad_region=6309, passed=41372
Got 41372 stars (including 33618 good ones) from the SExtractor catalog wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat
util/solve_plate_with_UCAC5 got 41372 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 980 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 35715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 35715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 35715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits N_match=980 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.308 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.332 n_q1=319 n_q2=190 n_q3=284 n_q4=187 worst_quadrant_to_overall_ratio=1.208
The image catalog is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits -region wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.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.uiUABR2uhO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Checking if the catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
WCS catalog name: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=60, bad_region=171, passed=4189
Got 4189 stars (including 3958 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat
util/solve_plate_with_UCAC5 got 4189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.2)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 3937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.2)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 3937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 3937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits N_match=951 sigma_overall_arcsec=0.583 sigma_q1_arcsec=0.495 sigma_q2_arcsec=0.703 sigma_q3_arcsec=0.634 sigma_q4_arcsec=0.709 n_q1=395 n_q2=108 n_q3=376 n_q4=72 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits -region wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.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.mi0dblkZpp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS-calibrated image found: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Checking if the catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat corresponding to the image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
WCS catalog name: wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=53, bad_region=163, passed=4401
Got 4401 stars (including 4187 good ones) from the SExtractor catalog wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 4401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 4101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 4103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 4103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits N_match=950 sigma_overall_arcsec=0.699 sigma_q1_arcsec=0.650 sigma_q2_arcsec=0.821 sigma_q3_arcsec=0.724 sigma_q4_arcsec=0.803 n_q1=373 n_q2=79 n_q3=447 n_q4=51 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits -region wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.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_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-09_20.00sec_5.00C_LIGHT_0238.fits
Saving fully-calibrated image wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-16_CI_Boo-03-Q2b1x1_033632_TTUQ2b1x1_2352489_67RzSKRl/wcs_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239.fits
Preparing the HTML report for the field Boo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:47:14.71 +48:13:37.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:40.38 +48:13:32.5: 11.80 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:22.81 +48:03:08.3: 13.22 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:35:13.78 +42:18:51.2: 12.75 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:18.41 +48:26:55.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:58:58.19 +47:13:43.3: 12.80 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:30.04 +47:55:26.3: 12.75 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:57:21.97 +47:41:19.0: 12.56 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:36.21 +42:03:25.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:37:54.34 +49:51:39.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:47:14.71 +48:13:37.7: 13.63 +/- 0.04 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:22.81 +48:03:08.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:30.04 +47:55:26.3: 12.72 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:40.38 +48:13:32.5: 11.80 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:35:13.78 +42:18:51.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:18.41 +48:26:55.8: 13.32 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:58:58.19 +47:13:43.3: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:37:54.34 +49:51:39.8: 12.83 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:57:21.97 +47:41:19.0: 12.57 +/- 0.01 detection
Forced photometry filter KEPT candidate at 15:47:14.71 +48:13:37.7: ref_mag=13.60 +/- 0.02 new_mean_mag=12.2370 delta=1.36 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:36.21 +42:03:25.8: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry reference-image weighted average: 11.80 +/- 0.00
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 15:53:22.81 +48:03:08.3: ref_mag=13.24 +/- 0.02 new_mean_mag=11.9731 delta=1.27 (need > 0.90)
Forced photometry filter KEPT candidate at 15:53:40.38 +48:13:32.5: ref_mag=11.80 +/- 0.00 new_mean_mag=10.8749 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 15:35:13.78 +42:18:51.2: ref_mag=12.78 +/- 0.01 new_mean_mag=11.6007 delta=1.18 (need > 0.90)
Forced photometry filter KEPT candidate at 15:53:18.41 +48:26:55.8: ref_mag=13.36 +/- 0.02 new_mean_mag=12.1259 delta=1.23 (need > 0.90)
Forced photometry filter KEPT candidate at 15:51:30.04 +47:55:26.3: ref_mag=12.73 +/- 0.01 new_mean_mag=11.4130 delta=1.32 (need > 0.90)
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 15:58:58.19 +47:13:43.3: ref_mag=12.80 +/- 0.01 new_mean_mag=11.6560 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 15:57:21.97 +47:41:19.0: ref_mag=12.57 +/- 0.01 new_mean_mag=11.5877 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 15:37:54.34 +49:51:39.8: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8742 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 15:51:36.21 +42:03:25.8: ref_mag=13.11 +/- 0.02 new_mean_mag=11.8498 delta=1.26 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:17.54 +47:50:55.7: 13.37 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:17.54 +47:50:55.7: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 15:51:17.54 +47:50:55.7: ref_mag=13.40 +/- 0.02 new_mean_mag=12.1265 delta=1.28 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 16:01:27.09 +47:46:21.4: 13.38 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 16:01:27.09 +47:46:21.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 16:01:27.09 +47:46:21.4: ref_mag=13.40 +/- 0.02 new_mean_mag=12.0697 delta=1.33 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:46.93 +42:12:59.1: 12.41 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:46.93 +42:12:59.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 15:34:46.93 +42:12:59.1: ref_mag=12.41 +/- 0.01 new_mean_mag=11.4136 delta=0.99 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:38.14 +42:16:01.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:47:17.82 +48:06:04.0: 13.53 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:50:00.41 +48:35:36.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:38.14 +42:16:01.8: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 15:34:38.14 +42:16:01.8: ref_mag=13.38 +/- 0.02 new_mean_mag=12.0035 delta=1.38 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:47:17.82 +48:06:04.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter KEPT candidate at 15:47:17.82 +48:06:04.0: ref_mag=13.49 +/- 0.02 new_mean_mag=12.1698 delta=1.32 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:50:00.41 +48:35:36.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 15:50:00.41 +48:35:36.4: ref_mag=13.02 +/- 0.01 new_mean_mag=11.8616 delta=1.15 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:46:03.49 +47:55:51.4: 12.31 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:34.02 +48:09:18.0: 13.27 +/- 0.03 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:59:21.51 +47:08:04.2: 12.69 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:46:03.49 +47:55:51.4: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 15:46:03.49 +47:55:51.4: ref_mag=12.33 +/- 0.01 new_mean_mag=11.3905 delta=0.94 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:34.02 +48:09:18.0: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 15:53:34.02 +48:09:18.0: ref_mag=13.28 +/- 0.02 new_mean_mag=11.9619 delta=1.32 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:59:21.51 +47:08:04.2: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 15:59:21.51 +47:08:04.2: ref_mag=12.72 +/- 0.01 new_mean_mag=11.8109 delta=0.91 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:50:50.97 +48:09:37.0: 12.31 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:50:50.97 +48:09:37.0: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 15:50:50.97 +48:09:37.0: ref_mag=12.33 +/- 0.01 new_mean_mag=11.1885 delta=1.14 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:31.06 +48:11:32.6: 12.63 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:31.06 +48:11:32.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 15:53:31.06 +48:11:32.6: ref_mag=12.65 +/- 0.01 new_mean_mag=11.5495 delta=1.10 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:58.41 +42:20:30.4: 11.50 +/- 0.00 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 16:00:14.27 +46:04:07.3: 12.60 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:58.41 +42:20:30.4: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.00
Forced photometry filter KEPT candidate at 15:34:58.41 +42:20:30.4: ref_mag=11.50 +/- 0.00 new_mean_mag=10.4686 delta=1.03 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:53:14.91 +48:13:21.0: 12.25 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 16:00:14.27 +46:04:07.3: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 16:00:14.27 +46:04:07.3: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6450 delta=0.96 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:53:14.91 +48:13:21.0: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 15:53:14.91 +48:13:21.0: ref_mag=12.23 +/- 0.01 new_mean_mag=11.0844 delta=1.15 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 16:01:20.77 +47:49:32.1: 12.59 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 16:01:20.77 +47:49:32.1: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 16:01:20.77 +47:49:32.1: ref_mag=12.56 +/- 0.01 new_mean_mag=11.6417 delta=0.92 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:27.08 +47:41:07.5: 12.19 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:27.08 +47:41:07.5: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter KEPT candidate at 15:51:27.08 +47:41:07.5: ref_mag=12.18 +/- 0.01 new_mean_mag=11.0992 delta=1.08 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:46:51.41 +48:12:24.9: 12.15 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:34:38.64 +42:17:37.6: 12.11 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:46:51.41 +48:12:24.9: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter KEPT candidate at 15:46:51.41 +48:12:24.9: ref_mag=12.15 +/- 0.01 new_mean_mag=11.1804 delta=0.97 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:34:38.64 +42:17:37.6: 12.08 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:45:47.56 +48:24:50.6: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter KEPT candidate at 15:34:38.64 +42:17:37.6: ref_mag=12.10 +/- 0.01 new_mean_mag=10.9473 delta=1.15 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:45:47.56 +48:24:50.6: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter KEPT candidate at 15:45:47.56 +48:24:50.6: ref_mag=12.11 +/- 0.01 new_mean_mag=10.9693 delta=1.14 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:45:43.11 +48:32:07.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:45:43.11 +48:32:07.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 15:45:43.11 +48:32:07.6: ref_mag=12.93 +/- 0.01 new_mean_mag=11.7909 delta=1.14 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:59:20.93 +47:14:04.7: 11.97 +/- 0.01 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:50:56.32 +48:08:36.8: 13.20 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:44:15.57 +48:12:45.8: 12.90 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:59:20.93 +47:14:04.7: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 15:59:20.93 +47:14:04.7: ref_mag=11.96 +/- 0.01 new_mean_mag=10.9566 delta=1.00 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:50:56.32 +48:08:36.8: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 15:50:56.32 +48:08:36.8: ref_mag=13.19 +/- 0.02 new_mean_mag=11.8636 delta=1.32 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:44:15.57 +48:12:45.8: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 15:44:15.57 +48:12:45.8: ref_mag=12.89 +/- 0.01 new_mean_mag=11.6493 delta=1.24 (need > 0.90)
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-07_20.00sec_5.00C_LIGHT_0217.fits at 15:51:16.93 +47:37:53.0: 13.17 +/- 0.02 detection
Forced photometry on wcs_Boo-03-Q2b1x1_2026-06-08_01-47-49_20.00sec_4.90C_LIGHT_0218.fits at 15:51:16.93 +47:37:53.0: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 15:51:16.93 +47:37:53.0: ref_mag=13.20 +/- 0.02 new_mean_mag=11.9388 delta=1.26 (need > 0.90)
Adding exclusion_list_local.txt__out05066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33326.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 50s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 21s
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Considering the candidate 11868_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11868_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 13142_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 13142_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11382_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11382_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11099_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11099_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 05066_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 05066_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 14920_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 14920_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 33123_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 33123_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 12503_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 12503_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 32553_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 32553_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 10325_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 10325_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 12818_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 12818_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 12621_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 12621_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 32716_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 32716_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 32973_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 32973_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11909_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11909_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 09861_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 09861_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 12652_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 12652_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11455_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11455_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 15293_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 15293_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11533_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11533_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11274_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11274_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 33326_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 33326_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 19710_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 19710_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11164_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11164_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 12396_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 12396_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 13326_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 13326_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11445_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11445_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 33133_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 33133_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 10655_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 10655_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 10843_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
The candidate 10843_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239 did not pass the final checks
Rejecting candidate due to large distance (39.4") between the two second-epoch detections
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Considering the candidate 10208_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 10208_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 14839_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 14839_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11631_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11631_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 11521_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 11521_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
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Considering the candidate 13658_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
Preparing report for the candidate 13658_fd_Boo-03-Q2b1x1_2026-07-16_03-35-52_20.00sec_5.00C_LIGHT_0239
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 74s
Prepared the HTML report for the field Boo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
15:37:54.34 +49:51:39.8
15:50:00.41 +48:35:36.4
15:45:43.11 +48:32:07.6
15:53:18.41 +48:26:55.8
15:45:47.56 +48:24:50.6
15:53:40.38 +48:13:32.5
15:53:14.91 +48:13:21.0
15:53:31.06 +48:11:32.6
15:47:14.71 +48:13:37.7
15:46:51.41 +48:12:24.9
15:53:34.02 +48:09:18.0
15:44:15.57 +48:12:45.8
15:50:50.97 +48:09:37.0
15:50:56.32 +48:08:36.8
15:53:22.81 +48:03:08.3
15:47:17.82 +48:06:04.0
16:01:20.77 +47:49:32.1
15:51:30.04 +47:55:26.3
16:01:27.09 +47:46:21.4
15:46:03.49 +47:55:51.4
15:51:17.54 +47:50:55.7
15:57:21.97 +47:41:19.0
15:51:27.08 +47:41:07.5
15:51:16.93 +47:37:53.0
15:59:20.93 +47:14:04.7
15:58:58.19 +47:13:43.3
15:59:21.51 +47:08:04.2
16:00:14.27 +46:04:07.3
15:51:36.21 +42:03:25.8
15:34:46.93 +42:12:59.1
15:34:38.14 +42:16:01.8
15:35:13.78 +42:18:51.2
15:34:38.64 +42:17:37.6
15:34:58.41 +42:20:30.4
########### Completed Boo-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
15:53:22.81 +48:03:08.3
15:57:21.97 +47:41:19.0
15:47:14.71 +48:13:37.7
15:53:40.38 +48:13:32.5
15:37:54.34 +49:51:39.8
15:58:58.19 +47:13:43.3
15:35:13.78 +42:18:51.2
15:51:30.04 +47:55:26.3
15:51:36.21 +42:03:25.8
15:53:18.41 +48:26:55.8
15:51:17.54 +47:50:55.7
16:01:27.09 +47:46:21.4
15:34:46.93 +42:12:59.1
15:34:38.14 +42:16:01.8
15:47:17.82 +48:06:04.0
15:50:00.41 +48:35:36.4
15:46:03.49 +47:55:51.4
15:53:34.02 +48:09:18.0
15:59:21.51 +47:08:04.2
15:50:50.97 +48:09:37.0
15:53:31.06 +48:11:32.6
15:34:58.41 +42:20:30.4
16:00:14.27 +46:04:07.3
15:53:14.91 +48:13:21.0
16:01:20.77 +47:49:32.1
15:51:27.08 +47:41:07.5
15:46:51.41 +48:12:24.9
15:34:38.64 +42:17:37.6
15:45:47.56 +48:24:50.6
15:45:43.11 +48:32:07.6
15:59:20.93 +47:14:04.7
15:50:56.32 +48:08:36.8
15:44:15.57 +48:12:45.8
15:51:16.93 +47:37:53.0
###################################################################################
15:53:22.81 +48:03:08.3 -- not an asteroid (will add it to exclusion list)
15:57:21.97 +47:41:19.0 -- not an asteroid (will add it to exclusion list)
15:47:14.71 +48:13:37.7 -- not an asteroid (will add it to exclusion list)
15:53:40.38 +48:13:32.5 -- not an asteroid (will add it to exclusion list)
15:37:54.34 +49:51:39.8 -- not an asteroid (will add it to exclusion list)
15:58:58.19 +47:13:43.3 -- not an asteroid (will add it to exclusion list)
15:35:13.78 +42:18:51.2 -- not an asteroid (will add it to exclusion list)
15:51:30.04 +47:55:26.3 -- not an asteroid (will add it to exclusion list)
15:51:36.21 +42:03:25.8 -- not an asteroid (will add it to exclusion list)
15:53:18.41 +48:26:55.8 -- not an asteroid (will add it to exclusion list)
15:51:17.54 +47:50:55.7 -- not an asteroid (will add it to exclusion list)
16:01:27.09 +47:46:21.4 -- not an asteroid (will add it to exclusion list)
15:34:46.93 +42:12:59.1 -- not an asteroid (will add it to exclusion list)
15:34:38.14 +42:16:01.8 -- not an asteroid (will add it to exclusion list)
15:47:17.82 +48:06:04.0 -- not an asteroid (will add it to exclusion list)
15:50:00.41 +48:35:36.4 -- not an asteroid (will add it to exclusion list)
15:46:03.49 +47:55:51.4 -- not an asteroid (will add it to exclusion list)
15:53:34.02 +48:09:18.0 -- not an asteroid (will add it to exclusion list)
15:59:21.51 +47:08:04.2 -- not an asteroid (will add it to exclusion list)
15:50:50.97 +48:09:37.0 -- not an asteroid (will add it to exclusion list)
15:53:31.06 +48:11:32.6 -- not an asteroid (will add it to exclusion list)
15:34:58.41 +42:20:30.4 -- not an asteroid (will add it to exclusion list)
16:00:14.27 +46:04:07.3 -- not an asteroid (will add it to exclusion list)
15:53:14.91 +48:13:21.0 -- not an asteroid (will add it to exclusion list)
16:01:20.77 +47:49:32.1 -- not an asteroid (will add it to exclusion list)
15:51:27.08 +47:41:07.5 -- not an asteroid (will add it to exclusion list)
15:46:51.41 +48:12:24.9 -- not an asteroid (will add it to exclusion list)
15:34:38.64 +42:17:37.6 -- not an asteroid (will add it to exclusion list)
15:45:47.56 +48:24:50.6 -- not an asteroid (will add it to exclusion list)
15:45:43.11 +48:32:07.6 -- not an asteroid (will add it to exclusion list)
15:59:20.93 +47:14:04.7 -- not an asteroid (will add it to exclusion list)
15:50:56.32 +48:08:36.8 -- not an asteroid (will add it to exclusion list)
15:44:15.57 +48:12:45.8 -- not an asteroid (will add it to exclusion list)
15:51:16.93 +47:37:53.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
15:34:38.14 +42:16:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:38.64 +42:17:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:46.93 +42:12:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:58.41 +42:20:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:35:13.78 +42:18:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:37:54.34 +49:51:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:15.57 +48:12:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:43.11 +48:32:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:47.56 +48:24:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:03.49 +47:55:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:51.41 +48:12:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:14.71 +48:13:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:17.82 +48:06:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:00.41 +48:35:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:50.97 +48:09:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:56.32 +48:08:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:16.93 +47:37:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:17.54 +47:50:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:27.08 +47:41:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:30.04 +47:55:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:36.21 +42:03:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:14.91 +48:13:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:18.41 +48:26:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:22.81 +48:03:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:31.06 +48:11:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:34.02 +48:09:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:40.38 +48:13:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:21.97 +47:41:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:58:58.19 +47:13:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:20.93 +47:14:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:21.51 +47:08:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:00:14.27 +46:04:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:01:20.77 +47:49:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:01:27.09 +47:46:21.4 -- 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)
15:34:38.14 +42:16:01.8 -- not a known variable star
15:34:38.64 +42:17:37.6 -- not a known variable star
15:34:46.93 +42:12:59.1 -- not a known variable star
15:34:58.41 +42:20:30.4 -- not a known variable star
15:35:13.78 +42:18:51.2 -- not a known variable star
15:37:54.34 +49:51:39.8 -- not a known variable star
15:44:15.57 +48:12:45.8 -- not a known variable star
15:45:43.11 +48:32:07.6 -- not a known variable star
15:45:47.56 +48:24:50.6 -- not a known variable star
15:46:03.49 +47:55:51.4 -- not a known variable star
15:46:51.41 +48:12:24.9 -- not a known variable star
15:47:14.71 +48:13:37.7 -- a known variable star
15:47:17.82 +48:06:04.0 -- not a known variable star
15:50:00.41 +48:35:36.4 -- a known variable star
15:50:50.97 +48:09:37.0 -- not a known variable star
15:50:56.32 +48:08:36.8 -- not a known variable star
15:51:16.93 +47:37:53.0 -- not a known variable star
15:51:17.54 +47:50:55.7 -- not a known variable star
15:51:27.08 +47:41:07.5 -- not a known variable star
15:51:30.04 +47:55:26.3 -- a known variable star
15:51:36.21 +42:03:25.8 -- not a known variable star
15:53:14.91 +48:13:21.0 -- not a known variable star
15:53:18.41 +48:26:55.8 -- not a known variable star
15:53:22.81 +48:03:08.3 -- not a known variable star
15:53:31.06 +48:11:32.6 -- not a known variable star
15:53:34.02 +48:09:18.0 -- not a known variable star
15:53:40.38 +48:13:32.5 -- not a known variable star
15:57:21.97 +47:41:19.0 -- not a known variable star
15:58:58.19 +47:13:43.3 -- not a known variable star
15:59:20.93 +47:14:04.7 -- not a known variable star
15:59:21.51 +47:08:04.2 -- a known variable star
16:00:14.27 +46:04:07.3 -- not a known variable star
16:01:20.77 +47:49:32.1 -- not a known variable star
16:01:27.09 +47:46:21.4 -- not a known variable star
Found 30 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
34 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 ####
15:34:38.14 +42:16:01.8
15:34:38.64 +42:17:37.6
15:34:46.93 +42:12:59.1
15:34:58.41 +42:20:30.4
15:35:13.78 +42:18:51.2
15:37:54.34 +49:51:39.8
15:44:15.57 +48:12:45.8
15:45:43.11 +48:32:07.6
15:45:47.56 +48:24:50.6
15:46:03.49 +47:55:51.4
15:46:51.41 +48:12:24.9
15:47:14.71 +48:13:37.7
15:47:17.82 +48:06:04.0
15:50:00.41 +48:35:36.4
15:50:50.97 +48:09:37.0
15:50:56.32 +48:08:36.8
15:51:16.93 +47:37:53.0
15:51:17.54 +47:50:55.7
15:51:27.08 +47:41:07.5
15:51:30.04 +47:55:26.3
15:51:36.21 +42:03:25.8
15:53:14.91 +48:13:21.0
15:53:18.41 +48:26:55.8
15:53:22.81 +48:03:08.3
15:53:31.06 +48:11:32.6
15:53:34.02 +48:09:18.0
15:53:40.38 +48:13:32.5
15:57:21.97 +47:41:19.0
15:58:58.19 +47:13:43.3
15:59:20.93 +47:14:04.7
15:59:21.51 +47:08:04.2
16:00:14.27 +46:04:07.3
16:01:20.77 +47:49:32.1
16:01:27.09 +47:46:21.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461237.85786345 -observatory V36
07:16:34.50 +17:18:12.2 Mercury (4.8mag)
10:36:23.83 +09:58:48.9 Venus (-4.1mag)
04:41:58.93 +22:06:42.1 Mars (1.3mag)
08:22:08.71 +19:53:56.0 Jupiter (-1.8mag)
00:56:23.92 +03:22:06.6 Saturn (0.7mag)
04:08:20.75 +20:48:02.7 Uranus (5.8mag)
00:16:57.74 +00:19:56.3 Neptune (7.7mag)
20:30:21.27 -23:20:39.2 Pluto (14.4mag)
09:32:01.94 +14:46:01.5 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Jul 16 03:51 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461237.85786345:
08:22:08.22 +19:53:57.2 Io (6.0mag)
08:22:00.21 +19:54:29.3 Europa (6.3mag)
08:22:14.77 +19:53:37.2 Ganymede (5.6mag)
08:21:45.57 +19:55:21.7 Callisto (6.8mag)
08:20:24.23 +19:40:44.5 Himalia (15.7mag)
08:22:06.88 +19:54:04.0 Thebe (16.6mag)
08:19:45.00 +19:43:52.9 Elara (17.7mag)
08:25:51.49 +19:44:54.0 Pasiphae (17.9mag)
08:26:45.70 +19:59:54.8 Carme (19.0mag)
00:56:35.84 +03:21:52.4 Titan (8.5mag)
00:56:26.25 +03:21:51.7 Rhea (9.8mag)
00:55:49.13 +03:20:12.7 Iapetus (11.2mag)
00:56:10.54 +03:22:18.0 Hyperion (14.5mag)
00:56:16.61 +03:18:28.0 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 16 03:52 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461237.85786345:
17:54:55.60 -31:34:17.3 JWST
17:42:11.46 +35:05:05.3 Chandra
04:25:00.51 +53:48:20.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 16 03:51 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461237.85786345 -observatory V36
02:44:42.23 +15:07:37.4 17.8mag P/1996 R2 (Lagerkvist)
18:13:28.72 -34:30:29.9 13.8mag P/2010 H2 (Vales)
06:31:40.41 -68:14:44.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:02:52.10 +32:33:02.9 17.6mag C/2017 K2 (PANSTARRS)
02:19:18.79 +18:36:42.0 15.7mag P/2021 N1 (ZTF)
22:55:47.00 +32:15:00.8 17.3mag C/2022 E2 (ATLAS)
06:19:12.18 +26:52:05.7 16.7mag C/2022 N2 (PANSTARRS)
10:00:47.14 +29:30:38.7 16.9mag C/2022 QE78 (ATLAS)
09:13:38.15 +05:06:17.2 17.9mag C/2022 R6 (PANSTARRS)
18:03:38.22 +21:02:35.1 18.0mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:07.32 -11:32:01.8 17.8mag P/2023 B1 (PANSTARRS)
21:41:45.95 +67:32:12.3 17.8mag C/2023 H5 (Lemmon)
16:19:32.31 -10:42:05.0 14.0mag C/2023 R1 (PANSTARRS)
08:11:11.65 +66:02:21.5 17.9mag C/2024 A1 (ATLAS)
07:40:36.29 +30:18:10.5 14.8mag C/2024 E1 (Wierzchos)
15:13:35.31 +15:28:00.8 17.6mag C/2024 G6 (ATLAS)
19:33:31.88 +40:29:58.8 13.7mag C/2024 J3 (ATLAS)
21:41:05.83 +46:52:27.6 17.8mag C/2024 R4 (PANSTARRS)
04:55:15.83 -13:32:26.9 15.7mag C/2024 T5 (ATLAS)
06:39:29.25 +28:04:00.7 18.0mag C/2025 J1 (Borisov)
07:18:25.79 -13:26:41.8 16.8mag C/2025 R3 (PANSTARRS)
10:03:10.67 +22:10:08.4 17.6mag C/2025 V2 (Rankin)
12:46:45.97 +03:40:04.6 17.1mag C/2025 Y1 (ATLAS)
16:35:43.51 +79:09:29.8 17.2mag C/2026 A2 (Bok)
02:52:21.17 +45:29:28.3 16.8mag C/2026 B2 (Sun-Gao)
11:29:27.12 +05:33:54.5 17.0mag A/2026 E1
21:28:17.98 -17:20:18.0 7.1mag 10P/Tempel
11:16:20.81 -02:09:14.5 16.2mag 29P/Schwassmann-Wachmann
04:08:45.99 +30:11:52.6 17.9mag 47P/Ashbrook-Jackson
10:20:36.37 +12:05:21.7 17.1mag 63P/Wild
00:50:45.26 -05:02:51.5 15.5mag 65P/Gunn
04:41:53.95 +20:27:25.2 13.7mag 78P/Gehrels
02:31:48.49 +11:24:31.2 16.3mag 88P/Howell
06:53:15.49 +30:08:06.8 15.8mag 93P/Lovas
04:40:36.40 +31:18:30.4 16.7mag 114P/Wiseman-Skiff
08:23:22.24 +30:00:19.5 15.2mag 123P/West-Hartley
10:59:23.48 -01:14:57.0 16.9mag 124P/Mrkos
05:01:20.79 +20:58:10.4 16.2mag 128P/Shoemaker-Holt
05:47:31.99 +19:38:47.4 17.8mag 131P/Mueller
00:02:58.70 +03:08:56.3 17.9mag 139P/Vaisala-Oterma
07:35:09.89 +15:41:39.1 16.3mag 141P-D/Machholz
03:19:10.70 -20:37:36.8 15.2mag 161P/Hartley-IRAS
05:54:44.11 +35:09:30.6 15.4mag 162P/SidingSpring
18:46:33.99 +19:04:06.5 14.2mag 169P/NEAT
01:55:11.46 +08:13:53.3 17.6mag 220P/McNaught
16:35:30.08 -08:38:49.9 17.2mag 235P/LINEAR
08:57:52.85 +32:43:50.8 18.0mag 240P/NEAT
20:39:08.48 -50:48:12.3 17.8mag 259P/Garradd
02:16:11.97 +14:54:08.8 15.6mag 260P/McNaught
05:55:30.66 +37:16:33.8 17.4mag 295P/LINEAR
15:06:29.48 +05:30:27.8 17.6mag 391P/Kowalski
08:40:01.10 +19:25:41.6 17.9mag 450P/LONEOS
08:01:09.89 +38:42:50.4 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.6K Jul 16 03:52 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
11:06:55.46 -04:07:04.50 2026-07-5.01 16.82
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
-rw-r--r-- 1 apache apache 5.6K Jul 16 03:51 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
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
-rw-r--r-- 1 apache apache 189K Jul 16 03:51 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:58:49.786 -21:29:54.27 AT 2026ssv 2026-07-06.26 21.93
21:15:32.626 -21:37:53.76 AT 2026ssu 2026-06-27.33 21.39
22:49:45.273 -15:16:33.71 AT 2026sst 2026-06-27.41 21.88
22:21:22.865 -18:28:38.60 AT 2026sss 2026-06-26.37 22.73
21:48:11.294 -15:58:33.77 AT 2026ssr 2026-06-26.41 21.95
21:56:29.244 -10:33:36.38 AT 2026ssq 2026-06-26.39 22.31
22:04:36.634 -18:37:38.63 AT 2026ssp 2026-06-26.37 22.56
21:52:03.725 -20:04:23.97 AT 2026sso 2026-06-26.39 22.15
22:28:31.768 -14:13:03.02 AT 2026ssn 2026-06-26.40 23.19
22:10:38.868 -20:00:07.81 AT 2026ssm 2026-06-26.37 21.5
00:37:08.843 -05:37:20.31 AT 2026ssl 2026-06-23.58 20.49
16:50:39.367 +12:02:04.48 AT 2026ssk 2026-06-23.30 21.04
21:28:51.588 -30:52:46.37 AT 2026ssj 2026-06-23.54 20.48
13:14:31.067 +38:32:01.92 AT 2026ssi 2026-06-11.32 19.048
00:23:13.025 -04:43:14.99 AT 2026ssh 2026-06-23.58 20.7
21:26:53.186 +04:17:24.51 AT 2026ssg 2026-06-23.48 20.92
22:34:24.397 -29:59:37.51 AT 2026ssf 2026-06-25.56 20.68
22:26:15.310 -27:42:10.55 AT 2026sse 2026-06-25.56 21.41
22:13:00.422 -28:48:04.48 AT 2026ssd 2026-06-25.55 21.47
22:13:31.243 -26:34:31.26 AT 2026ssc 2026-06-25.55 21.32
-rw-r--r-- 1 apache apache 89K Jul 16 03:51 tns_transients_list.txt
