This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF
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 18.2507 2461239.7507 9.57 20:00:28.72 +01:11:10.4
42.07655 -14.74830 galactic Aql Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237688379494570752 | 20:00:28.72 +01:11:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1949AnHar.112....1C HD 357759 J-Ks=0.335+/-0.039 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:28.72 +01:11:10.4: 10.57 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:28.72 +01:11:10.4: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 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 4237688379494570752,2461239.7507,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4237688379494570752 20260718.2507 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 9.88 20:00:32.05 +01:38:59.3
42.50429 -14.53893 galactic Aql Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237743458157008640 | 20:00:32.04 +01:38:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 357758 J-Ks=0.454+/-0.033 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:32.05 +01:38:59.3: 10.74 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:32.05 +01:38:59.3: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 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 4237743458157008640,2461239.7507,9.88,0.05,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 4237743458157008640 20260718.2507 9.88CV 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 18.2507 2461239.7507 9.96 20:00:15.18 +01:02:31.9
41.91782 -14.76738 galactic Aql Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237638008117089792 | 20:00:15.16 +01:02:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 357766 J-Ks=0.299+/-0.033 (F)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:15.18 +01:02:31.9: 10.92 +/- 0.01 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:15.18 +01:02:31.9: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 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 4237638008117089792,2461239.7507,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4237638008117089792 20260718.2507 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.38 20:00:34.83 +01:24:24.7
42.28954 -14.66531 galactic Aql Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.1450+01.4068 | 20:00:34.83 +01:24:24.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.667+/-0.030 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:34.83 +01:24:24.7: 13.69 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:34.83 +01:24:24.7: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1450+01.4068,2461239.7507,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1450+01.4068 20260718.2507 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.16 19:59:16.31 +01:12:20.5
41.94562 -14.47386 galactic Aql Second-epoch detections are separated by 1.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:59:16.31 +01:12:20.5 (user input) | T | P | (position from user input) J-Ks=0.759+/-0.030 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:16.31 +01:12:20.5: 13.16 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:16.31 +01:12:20.5: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,12.16,0.05,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
target 20260718.2507 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 18.2507 2461239.7507 12.47 20:00:22.93 +00:57:56.6
41.86418 -14.83219 galactic Aql Second-epoch detections are separated by 1.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0980+00.9671 | 20:00:22.93 +00:57:56.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.433+/-0.033 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:22.93 +00:57:56.6: 13.55 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:22.93 +00:57:56.6: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0980+00.9671,2461239.7507,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0980+00.9671 20260718.2507 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.62 20:00:16.32 +01:07:02.2
41.98842 -14.73577 galactic Aql Second-epoch detections are separated by 2.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:16.32 +01:07:02.2 (user input) | T | P | (position from user input) J-Ks=0.998+/-0.031 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:16.32 +01:07:02.2: 13.79 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:16.32 +01:07:02.2: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.62,0.05,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 20260718.2507 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.45 20:00:02.99 +00:55:57.6
41.79320 -14.77488 galactic Aql Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0049+00.9345 | 20:00:02.99 +00:55:57.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.925+/-0.033 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:02.99 +00:55:57.6: 13.56 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:02.99 +00:55:57.6: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0049+00.9345,2461239.7507,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0049+00.9345 20260718.2507 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.21 19:26:09.21 -04:06:02.2
33.22181 -9.58781 galactic Aql Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4211914585688359808 | 19:26:09.21 -04:06:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.188+/-0.043 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:26:09.21 -04:06:02.2: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:26:09.21 -04:06:02.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 4211914585688359808,2461239.7507,12.21,0.05,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 4211914585688359808 20260718.2507 12.21CV 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 18.2507 2461239.7507 12.44 20:00:09.00 +01:30:04.5
42.32208 -14.52569 galactic Aql Second-epoch detections are separated by 1.6" and 8.3 pix
The object was found in VSX 2" ASASSN-V J200009.14+013005.7
Type: SRS
# Max. Min./Amp. JD0 Period
13.710 V 13.800 V 2457172.93000 15.696000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:09.00 +01:30:04.5: 13.56 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:09.00 +01:30:04.5: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200009.14+013005.7,2461239.7507,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200009.14+013005.7 20260718.2507 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.48 20:00:21.46 +01:47:45.5
42.61500 -14.43021 galactic Aql Second-epoch detections are separated by 0.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0893+01.7959 | 20:00:21.46 +01:47:45.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.533+/-0.036 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:21.46 +01:47:45.5: 13.43 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:21.46 +01:47:45.5: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0893+01.7959,2461239.7507,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0893+01.7959 20260718.2507 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.71 20:00:30.60 +01:13:50.3
42.12078 -14.73398 galactic Aql Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:30.60 +01:13:50.3 (user input) | T | P | (position from user input) J-Ks=0.699+/-0.035 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:30.60 +01:13:50.3: 12.87 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:30.60 +01:13:50.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.25 20:00:15.30 +01:10:07.3
42.03305 -14.70752 galactic Aql Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:15.30 +01:10:07.3 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:15.30 +01:10:07.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:15.30 +01:10:07.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.25,0.05,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 20260718.2507 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.88 20:00:14.77 +01:04:29.3
41.94662 -14.75034 galactic Aql Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0713+01.0554 | 20:00:16.44 +01:03:58.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.470+/-0.033 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:14.77 +01:04:29.3: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:14.77 +01:04:29.3: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J300.0713+01.0554,2461239.7507,11.88,0.05,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
ATO J300.0713+01.0554 20260718.2507 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 18.2507 2461239.7507 12.31 19:59:15.11 +01:05:37.4
41.84146 -14.52279 galactic Aql Second-epoch detections are separated by 1.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:59:15.11 +01:05:37.4 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.034 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:15.11 +01:05:37.4: 13.28 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:15.11 +01:05:37.4: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.31,0.05,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 20260718.2507 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.32 19:58:53.83 +01:02:57.3
41.75749 -14.46599 galactic Aql Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.7241+01.0605 | 19:58:53.83 +01:02:57.3 (user input) | DBF (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.358+/-0.043 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:53.83 +01:02:57.3: 13.29 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:53.83 +01:02:57.3: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7241+01.0605,2461239.7507,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7241+01.0605 20260718.2507 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.79 20:00:37.90 +01:40:24.1
42.53771 -14.54904 galactic Aql Second-epoch detections are separated by 0.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237743973552334080 | 20:00:37.90 +01:40:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.749+/-0.034 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.90 +01:40:24.1: 12.83 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.90 +01:40:24.1: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 4237743973552334080,2461239.7507,11.79,0.05,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
Gaia DR3 4237743973552334080 20260718.2507 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 18.2507 2461239.7507 12.15 20:00:02.22 +01:10:06.0
42.00586 -14.65980 galactic Aql Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:02.22 +01:10:06.0 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.033 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:02.22 +01:10:06.0: 13.10 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:02.22 +01:10:06.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,12.15,0.05,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 20260718.2507 12.15CV 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 18.2507 2461239.7507 11.62 20:00:27.76 +00:57:18.9
41.86456 -14.85487 galactic Aql Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237630552053772032 | 20:00:27.74 +00:57:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.365+/-0.033 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:27.76 +00:57:18.9: 12.56 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:27.76 +00:57:18.9: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 4237630552053772032,2461239.7507,11.62,0.05,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 4237630552053772032 20260718.2507 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.34 19:59:52.17 +00:57:56.4
41.80103 -14.71953 galactic Aql Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:59:52.17 +00:57:56.4 (user input) | T | P | (position from user input) J-Ks=0.768+/-0.032 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:52.17 +00:57:56.4: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:52.17 +00:57:56.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.34,0.05,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 20260718.2507 12.34CV 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 18.2507 2461239.7507 12.76 19:30:37.69 +01:15:00.0
38.55452 -8.13256 galactic Aql Second-epoch detections are separated by 1.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4287662626095191808 | 19:30:39.11 +01:14:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-0.032 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:30:37.69 +01:15:00.0: 13.76 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:30:37.69 +01:15:00.0: 13.74 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4287662626095191808,2461239.7507,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4287662626095191808 20260718.2507 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.46 20:00:36.05 +01:02:30.6
41.96034 -14.84399 galactic Aql Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237637458361237888 | 20:00:36.07 +01:02:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.844+/-0.030 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:36.05 +01:02:30.6: 12.54 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:36.05 +01:02:30.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 4237637458361237888,2461239.7507,11.46,0.05,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 4237637458361237888 20260718.2507 11.46CV 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 18.2507 2461239.7507 11.88 20:00:37.04 +01:43:48.7
42.58748 -14.51868 galactic Aql Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:37.04 +01:43:48.7 (user input) | T | P | (position from user input) J-Ks=0.752+/-0.033 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.04 +01:43:48.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.04 +01:43:48.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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,2461239.7507,11.88,0.05,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 20260718.2507 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 18.2507 2461239.7507 12.73 19:25:29.32 -03:52:42.8
33.34671 -9.33957 galactic Aql Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:25:29.32 -03:52:42.8 (user input) | T | P | (position from user input) J-Ks=0.527+/-0.032 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:29.32 -03:52:42.8: 13.69 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:29.32 -03:52:42.8: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.27 20:00:37.37 +00:54:01.6
41.83442 -14.91618 galactic Aql Second-epoch detections are separated by 0.7" and 8.6 pix
The object was found in VSX 1" Gaia DR3 4237626463244848512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.210 G 13.230 G A
The object was not found in astcheck.
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.37 +00:54:01.6: 13.24 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.37 +00:54:01.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4237626463244848512,2461239.7507,12.27,0.05,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 4237626463244848512 20260718.2507 12.27CV 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 18.2507 2461239.7507 12.38 20:00:18.84 +01:48:49.9
42.62581 -14.41206 galactic Aql Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:18.84 +01:48:49.9 (user input) | T | P | (position from user input) J-Ks=0.680+/-0.031 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:18.84 +01:48:49.9: 13.43 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:18.84 +01:48:49.9: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.86 19:59:38.95 +00:56:00.3
41.74461 -14.68643 galactic Aql Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237676319226752640 | 19:59:38.98 +00:56:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.034+/-0.035 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:38.95 +00:56:00.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:38.95 +00:56:00.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 4237676319226752640,2461239.7507,11.86,0.05,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
Gaia DR3 4237676319226752640 20260718.2507 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 18.2507 2461239.7507 12.27 19:25:35.50 -03:48:20.0
33.42447 -9.32948 galactic Aql Second-epoch detections are separated by 1.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.3941-03.8077 | 19:25:35.50 -03:48:20.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7IV (LAMOST DR5) J-Ks=0.304+/-0.033 (F)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:35.50 -03:48:20.0: 13.22 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:35.50 -03:48:20.0: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.3941-03.8077,2461239.7507,12.27,0.05,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 J291.3941-03.8077 20260718.2507 12.27CV 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 18.2507 2461239.7507 11.51 20:00:00.95 +00:57:51.0
41.81767 -14.75241 galactic Aql Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237631376687560320 | 20:00:00.98 +00:57:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.773+/-0.035 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:00.95 +00:57:51.0: 12.46 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:00.95 +00:57:51.0: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 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 4237631376687560320,2461239.7507,11.51,0.05,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 4237631376687560320 20260718.2507 11.51CV 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 18.2507 2461239.7507 12.43 20:00:38.37 +01:01:10.3
41.94482 -14.86312 galactic Aql Second-epoch detections are separated by 1.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:38.37 +01:01:10.3 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.034 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:38.37 +01:01:10.3: 13.83 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:38.37 +01:01:10.3: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.72 20:00:16.40 +01:03:58.5
41.94219 -14.76039 galactic Aql Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0713+01.0554 | 20:00:16.44 +01:03:58.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.688+/-0.029 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:16.40 +01:03:58.5: 12.74 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:16.40 +01:03:58.5: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0713+01.0554,2461239.7507,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0713+01.0554 20260718.2507 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.39 19:58:34.56 +00:47:42.2
41.48708 -14.51614 galactic Aql Second-epoch detections are separated by 1.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:58:34.56 +00:47:42.2 (user input) | T | P | (position from user input) J-Ks=0.790+/-0.034 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:34.56 +00:47:42.2: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:34.56 +00:47:42.2: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.21 20:00:39.29 +01:09:59.8
42.08045 -14.79635 galactic Aql Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.1638+01.1668 | 20:00:39.33 +01:10:00.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.135+/-0.041 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:39.29 +01:09:59.8: 12.40 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:39.29 +01:09:59.8: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 J300.1638+01.1668,2461239.7507,11.21,0.05,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
ATO J300.1638+01.1668 20260718.2507 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 18.2507 2461239.7507 12.29 19:25:17.00 -04:56:56.1
32.35442 -9.77638 galactic Aql Second-epoch detections are separated by 1.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:25:17.00 -04:56:56.1 (user input) | T | P | (position from user input) J-Ks=0.878+/-0.031 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:17.00 -04:56:56.1: 13.21 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:17.00 -04:56:56.1: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.48 19:59:48.61 +01:14:06.1
42.03851 -14.57816 galactic Aql Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9485+01.2363 | 19:59:48.64 +01:14:06.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.011+/-0.033 (M)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:48.61 +01:14:06.1: 12.39 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:48.61 +01:14:06.1: 12.43 +/- 0.02 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
ATO J299.9485+01.2363,2461239.7507,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9485+01.2363 20260718.2507 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.08 19:58:32.62 +00:45:11.7
41.44510 -14.52887 galactic Aql Second-epoch detections are separated by 0.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:58:32.62 +00:45:11.7 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.042 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:32.62 +00:45:11.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:32.62 +00:45:11.7: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,12.08,0.05,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 20260718.2507 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.04 19:59:02.37 +00:55:12.4
41.65762 -14.55870 galactic Aql Second-epoch detections are separated by 1.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.7611+00.9162 | 19:59:02.37 +00:55:12.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.090+/-0.036 (A)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:02.37 +00:55:12.4: 12.97 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:02.37 +00:55:12.4: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7611+00.9162,2461239.7507,12.04,0.05,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
ATO J299.7611+00.9162 20260718.2507 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 18.2507 2461239.7507 12.13 20:00:11.41 +01:01:04.7
41.88805 -14.76511 galactic Aql Second-epoch detections are separated by 1.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:11.41 +01:01:04.7 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.032 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:11.41 +01:01:04.7: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:11.41 +01:01:04.7: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.03 19:58:46.79 +01:00:03.9
41.69933 -14.46310 galactic Aql Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:58:46.79 +01:00:03.9 (user input) | T | P | (position from user input) J-Ks=0.722+/-0.032 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:46.79 +01:00:03.9: 12.93 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:46.79 +01:00:03.9: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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,2461239.7507,12.03,0.05,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 20260718.2507 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 18.2507 2461239.7507 12.15 20:00:37.79 +01:08:29.4
42.05454 -14.80284 galactic Aql Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:37.79 +01:08:29.4 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.79 +01:08:29.4: 13.36 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.79 +01:08:29.4: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.15,0.05,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 20260718.2507 12.15CV 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 18.2507 2461239.7507 12.63 19:26:17.93 -04:19:09.7
33.04039 -9.71886 galactic Aql Second-epoch detections are separated by 1.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:26:17.93 -04:19:09.7 (user input) | T | P | (position from user input) J-Ks=0.543+/-0.035 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:26:17.93 -04:19:09.7: 13.66 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:26:17.93 -04:19:09.7: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.03 19:59:06.38 +00:57:11.0
41.69577 -14.55773 galactic Aql Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.7866+00.9578 | 19:59:06.38 +00:57:11.0 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.477+/-0.040 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:06.38 +00:57:11.0: 12.92 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:06.38 +00:57:11.0: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J299.7866+00.9578,2461239.7507,12.03,0.05,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
ATO J299.7866+00.9578 20260718.2507 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 18.2507 2461239.7507 12.19 19:59:29.79 +01:11:23.2
41.95880 -14.53081 galactic Aql Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:59:29.79 +01:11:23.2 (user input) | T | P | (position from user input) J-Ks=0.775+/-0.032 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:29.79 +01:11:23.2: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:29.79 +01:11:23.2: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.44 20:00:28.63 +01:46:53.5
42.61668 -14.46334 galactic Aql Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:28.63 +01:46:53.5 (user input) | T | P | (position from user input) J-Ks=0.542+/-0.035 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:28.63 +01:46:53.5: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:28.63 +01:46:53.5: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.38 19:59:13.43 +01:02:49.0
41.79552 -14.53890 galactic Aql Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.8021+01.0439 | 19:59:13.43 +01:02:49.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.457+/-0.033 (G)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:13.43 +01:02:49.0: 13.38 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:13.43 +01:02:49.0: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8021+01.0439,2461239.7507,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8021+01.0439 20260718.2507 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.62 19:59:58.29 +01:15:23.6
42.07794 -14.60333 galactic Aql Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4237692914980160640 | 19:59:58.30 +01:15:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.646+/-0.035 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:58.29 +01:15:23.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:58.29 +01:15:23.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 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 4237692914980160640,2461239.7507,11.62,0.05,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 4237692914980160640 20260718.2507 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 11.98 20:00:33.17 +01:07:23.8
42.02848 -14.79461 galactic Aql Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:33.17 +01:07:23.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:33.17 +01:07:23.8: 13.12 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:33.17 +01:07:23.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7507,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.53 19:25:21.42 -03:58:20.5
33.24687 -9.35267 galactic Aql Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.3399-03.9700 | 19:25:21.42 -03:58:20.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.727+/-0.041 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:21.42 -03:58:20.5: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:21.42 -03:58:20.5: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.3399-03.9700,2461239.7507,12.53,0.05,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 J291.3399-03.9700 20260718.2507 12.53CV 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 18.2507 2461239.7507 12.44 20:00:17.18 +01:16:44.0
42.13703 -14.66183 galactic Aql Second-epoch detections are separated by 1.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:17.18 +01:16:44.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:17.18 +01:16:44.0: 13.76 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:17.18 +01:16:44.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2507 2461239.7507 12.54 19:58:43.21 +00:51:05.3
41.55604 -14.52107 galactic Aql Second-epoch detections are separated by 1.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:58:43.21 +00:51:05.3 (user input) | T | P | (position from user input) J-Ks=0.771+/-0.035 (K)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:43.21 +00:51:05.3: 13.63 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:43.21 +00:51:05.3: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7507,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2507 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461208.87097431 17.06.2026 08:54:02.180 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
First image: 2461208.87097431 17.06.2026 08:54:02.180 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Last image: 2461239.75098417 18.07.2026 06:01:15.032 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
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: 29 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): 15961
Objects passed selection criteria: 15862
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: 9078.5
Average stars matched: 8492 (93.5397 %)
Memory usage VmPeak: 125056 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 04:14:10 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: 2461208.87097431 17.06.2026 08:54:02.180 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
First image: 2461208.87097431 17.06.2026 08:54:02.180 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Last image: 2461239.75098417 18.07.2026 06:01:15.032 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 70 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): 132865
Objects passed selection criteria: 132521
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 83156.5
Average stars matched: 73253.8 (88.0914 %)
Memory usage VmPeak: 1962852 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 04:23:35 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.cat to cache
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.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/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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: 2461239.75033411
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_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits exists and is non-empty
Saving wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits to local_wcs_cache/
'wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits' -> 'local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits'
wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits exists and is non-empty
Saving wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits to local_wcs_cache/
'wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits' -> 'local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits'
wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits exists and is non-empty
Saving wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits'
wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits exists and is non-empty
Saving wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits to local_wcs_cache/
'wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits (1st reference image)
verification OK: wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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: 19:42:50.503 -02:00:52.35 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_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Image size: 937.1'x624.1' 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: 19:42:51.731 -02:02:06.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:50.503 -02:00:52.35
Second-epoch image center 19:42:51.731 -02:02:06.37
Angular distance between the image centers 0.0212 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Image size: 937.2'x624.1' 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: 19:42:54.362 -02:02:36.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:50.503 -02:00:52.35
Second-epoch image center 19:42:54.362 -02:02:36.68
Angular distance between the image centers 0.0331 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 19:42:51.731 -02:02:06.37
Second-epoch second image center 19:42:54.362 -02:02:36.68
Angular distance between the image centers 0.01382 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/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits &> /tmp/tmp.L8PF34I1bW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits &> /tmp/tmp.vpXktZKfAL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits &> /tmp/tmp.1thwa8Akkm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits &> /tmp/tmp.v0zVWHheG8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits and wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits and wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits and wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat
The reference image (wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits) and catalog (wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat) found
'wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat' -> 'wcsmag.cat'
Read 21764 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8471 to 303.5886 deg, Dec -7.2732 to +3.2486 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 287.8471 to 303.5886 deg, Dec -7.2732 to 3.2486 deg
Loaded 10284 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): 8477 out of 8960 total matches.
Matched with Tycho-2 8960 out of 21764 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.807500
a=0.000000 b=1.000000 c=22.807500
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.97
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.97
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 21764 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8471 to 303.5886 deg, Dec -7.2732 to +3.2486 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 287.8471 to 303.5886 deg, Dec -7.2732 to 3.2486 deg
Loaded 10284 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): 8477 out of 8960 total matches.
Matched with Tycho-2 8960 out of 21764 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits:
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits (aperture=6.5)
Read 22168 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8676 to 303.6010 deg, Dec -7.2659 to +3.2601 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 287.8676 to 303.6010 deg, Dec -7.2659 to 3.2601 deg
Loaded 10285 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): 8462 out of 8967 total matches.
Matched with Tycho-2 8967 out of 22168 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits:
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.7 pix Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
2.5 pix Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
2.2 pix fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
2.2 pix fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
2.7 pix wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
2.5 pix wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Limiting magnitude estimates:
15.0 mag. Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
15.0 mag. Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
12.7 mag. fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
12.4 mag. fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.0 (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.L8PF34I1bW (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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=1351, bad_region=5458, passed=21764
Got 21764 stars (including 15342 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat
util/solve_plate_with_UCAC5 got 21764 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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 16719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 16719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 16719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits N_match=976 sigma_overall_arcsec=0.518 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.632 sigma_q3_arcsec=0.522 sigma_q4_arcsec=0.563 n_q1=332 n_q2=233 n_q3=249 n_q4=162 worst_quadrant_to_overall_ratio=1.220
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits -region wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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.vpXktZKfAL (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.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=1439, bad_region=6001, passed=22168
Got 22168 stars (including 15131 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat
util/solve_plate_with_UCAC5 got 22168 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits N_match=973 sigma_overall_arcsec=0.493 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.567 sigma_q3_arcsec=0.452 sigma_q4_arcsec=0.571 n_q1=325 n_q2=237 n_q3=240 n_q4=171 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits -region wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.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.1thwa8Akkm (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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=140, bad_region=195, passed=2490
Got 2490 stars (including 2160 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 2490 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 2279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits N_match=966 sigma_overall_arcsec=0.576 sigma_q1_arcsec=0.537 sigma_q2_arcsec=0.666 sigma_q3_arcsec=0.666 sigma_q4_arcsec=0.462 n_q1=455 n_q2=39 n_q3=376 n_q4=96 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits -region wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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.v0zVWHheG8 (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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=122, bad_region=73, passed=1879
Got 1879 stars (including 1686 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 1879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits N_match=960 sigma_overall_arcsec=0.615 sigma_q1_arcsec=0.610 sigma_q2_arcsec=0.516 sigma_q3_arcsec=0.715 sigma_q4_arcsec=0.461 n_q1=413 n_q2=36 n_q3=391 n_q4=120 worst_quadrant_to_overall_ratio=1.163
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits -region wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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=Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits sigma_overall=0.518 worst_q_ratio=1.220
ref2=Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits sigma_overall=0.493 worst_q_ratio=1.160
new1=fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits sigma_overall=0.576 worst_q_ratio=1.157
new2=fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits sigma_overall=0.615 worst_q_ratio=1.163
reference average sigma_overall=0.5055 worst_q_ratio=1.19
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389_astrometric_residuals.png (976 matched stars from wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369_astrometric_residuals.png (973 matched stars from wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212_astrometric_residuals.png (966 matched stars from wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213_astrometric_residuals.png (960 matched stars from wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits'
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits'
Preparing the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:15.18 +01:02:31.9: 10.92 +/- 0.01 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:32.05 +01:38:59.3: 10.74 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:28.72 +01:11:10.4: 10.57 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:32.05 +01:38:59.3: 10.78 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:28.72 +01:11:10.4: 10.58 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:15.18 +01:02:31.9: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Forced photometry filter KEPT candidate at 20:00:28.72 +01:11:10.4: ref_mag=10.57 +/- 0.00 new_mean_mag=9.5580 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 20:00:32.05 +01:38:59.3: ref_mag=10.76 +/- 0.00 new_mean_mag=9.8167 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 20:00:15.18 +01:02:31.9: ref_mag=10.91 +/- 0.00 new_mean_mag=9.9551 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out04387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05776.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05459_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 05459_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04387_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 04387_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05776_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 05776_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 22s
Prepared the HTML report for the field Aql-04-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 ####
20:00:32.05 +01:38:59.3
20:00:28.72 +01:11:10.4
20:00:15.18 +01:02:31.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.cat to cache
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Creating symlink local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits exists and is non-empty
wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits (1st reference image)
verification OK: wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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: 19:42:50.503 -02:00:52.35 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_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits (1st new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Image size: 937.1'x624.1' 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: 19:42:51.731 -02:02:06.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:50.503 -02:00:52.35
Second-epoch image center 19:42:51.731 -02:02:06.37
Angular distance between the image centers 0.0212 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits (2nd new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Image size: 937.2'x624.1' 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: 19:42:54.362 -02:02:36.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:50.503 -02:00:52.35
Second-epoch image center 19:42:54.362 -02:02:36.68
Angular distance between the image centers 0.0331 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 19:42:51.731 -02:02:06.37
Second-epoch second image center 19:42:54.362 -02:02:36.68
Angular distance between the image centers 0.01382 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/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits &> /tmp/tmp.y9zkDzTBPW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits &> /tmp/tmp.Wo2qD7tswV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits &> /tmp/tmp.OrE1aQioqy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits &> /tmp/tmp.Gdi4DfPNow
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits and wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits and wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits and wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat
The reference image (wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits) and catalog (wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat) found
'wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat' -> 'wcsmag.cat'
Read 156147 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8471 to 303.5886 deg, Dec -7.2775 to +3.2495 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 287.8471 to 303.5886 deg, Dec -7.2775 to 3.2495 deg
Loaded 10294 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): 7171 out of 9131 total matches.
Matched with Tycho-2 9131 out of 156147 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.666900
a=0.000000 b=1.000000 c=22.666900
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.12
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.12
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 156147 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8471 to 303.5886 deg, Dec -7.2775 to +3.2495 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 287.8471 to 303.5886 deg, Dec -7.2775 to 3.2495 deg
Loaded 10294 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): 7171 out of 9131 total matches.
Matched with Tycho-2 9131 out of 156147 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits:
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits (aperture=5.2)
Read 172469 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8642 to 303.6060 deg, Dec -7.2658 to +3.2606 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 287.8642 to 303.6060 deg, Dec -7.2658 to 3.2606 deg
Loaded 10290 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): 7119 out of 9160 total matches.
Matched with Tycho-2 9160 out of 172469 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits:
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 71 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.6 pix Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
2.4 pix Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
2.0 pix fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
2.1 pix fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
2.6 pix wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
2.4 pix wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Limiting magnitude estimates:
15.1 mag. Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
15.2 mag. Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
13.2 mag. fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
13.1 mag. fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.y9zkDzTBPW (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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=7, blended=19591, bad_region=29411, passed=156140
Got 156140 stars (including 112236 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat
util/solve_plate_with_UCAC5 got 156140 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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 128479 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 128477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 128477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits N_match=974 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.458 sigma_q2_arcsec=0.662 sigma_q3_arcsec=0.501 sigma_q4_arcsec=0.593 n_q1=343 n_q2=206 n_q3=267 n_q4=158 worst_quadrant_to_overall_ratio=1.314
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits -region wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.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.Wo2qD7tswV (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.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=14, blended=21576, bad_region=33209, passed=172455
Got 172455 stars (including 123076 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat
util/solve_plate_with_UCAC5 got 172455 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 141592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 141594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 141594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits N_match=976 sigma_overall_arcsec=0.483 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.489 sigma_q4_arcsec=0.573 n_q1=337 n_q2=213 n_q3=262 n_q4=164 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits -region wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.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.OrE1aQioqy (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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=12, blended=1704, bad_region=2884, passed=40769
Got 40769 stars (including 36179 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 40769 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 37465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 37465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 37465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits N_match=969 sigma_overall_arcsec=0.554 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.620 sigma_q3_arcsec=0.618 sigma_q4_arcsec=0.441 n_q1=451 n_q2=50 n_q3=363 n_q4=105 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits -region wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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.Gdi4DfPNow (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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1211, bad_region=1281, passed=32188
Got 32188 stars (including 29664 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 32188 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 30232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 30231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 30231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits N_match=964 sigma_overall_arcsec=0.613 sigma_q1_arcsec=0.632 sigma_q2_arcsec=0.588 sigma_q3_arcsec=0.681 sigma_q4_arcsec=0.446 n_q1=420 n_q2=42 n_q3=372 n_q4=130 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits -region wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-00-18_20.00sec_5.00C_LIGHT_0212.fits
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.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_2026-07-18_CI_Aql-04-Q2b1x1_021046_TTUQ2b1x1_3540075_0C4rQIiF/wcs_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213.fits
Preparing the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:35.92 +01:06:18.0: 11.98 +/- 0.01 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:33:50.45 +02:02:18.9: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:26:13.93 -03:35:56.6: 12.85 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:32:43.15 -05:19:53.7: 12.27 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:30:00.84 +01:17:46.5: 13.13 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:34:21.07 -00:36:48.9: 12.09 +/- 0.01 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:38.22 +00:34:33.1: 12.34 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:37:49.12 -02:25:59.2: 10.95 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:33:39.00 -04:10:57.8: 9.20 +/- 0.00 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:35.92 +01:06:18.0: 12.07 +/- 0.01 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:26:13.93 -03:35:56.6: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:33:50.45 +02:02:18.9: 12.67 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 19:59:35.92 +01:06:18.0: ref_mag=12.02 +/- 0.01 new_mean_mag=11.3435 delta=0.68 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:30:00.84 +01:17:46.5: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:38.22 +00:34:33.1: 12.43 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 19:26:13.93 -03:35:56.6: ref_mag=12.91 +/- 0.02 new_mean_mag=12.7747 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:32:43.15 -05:19:53.7: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Forced photometry filter REJECTED candidate at 19:33:50.45 +02:02:18.9: ref_mag=12.66 +/- 0.02 new_mean_mag=12.5716 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:30:00.84 +01:17:46.5: ref_mag=13.13 +/- 0.03 new_mean_mag=12.8739 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:34:21.07 -00:36:48.9: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 19:59:38.22 +00:34:33.1: ref_mag=12.38 +/- 0.01 new_mean_mag=12.1431 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:32:43.15 -05:19:53.7: ref_mag=12.33 +/- 0.01 new_mean_mag=12.3176 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 19:34:21.07 -00:36:48.9: ref_mag=12.13 +/- 0.01 new_mean_mag=12.6158 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:37:49.12 -02:25:59.2: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.00
Forced photometry filter REJECTED candidate at 19:37:49.12 -02:25:59.2: ref_mag=11.00 +/- 0.00 new_mean_mag=11.6532 delta=-0.65 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:33:39.00 -04:10:57.8: 9.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.22 +/- 0.00
Forced photometry filter REJECTED candidate at 19:33:39.00 -04:10:57.8: ref_mag=9.22 +/- 0.00 new_mean_mag=9.9691 delta=-0.75 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:27:16.09 +01:58:45.4: 12.25 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:27:16.09 +01:58:45.4: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter REJECTED candidate at 19:27:16.09 +01:58:45.4: ref_mag=12.27 +/- 0.01 new_mean_mag=12.1874 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:34.83 +01:24:24.7: 13.69 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:57:37.72 -00:00:11.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:16.31 +01:12:20.5: 13.16 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:22.93 +00:57:56.6: 13.55 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:16.32 +01:07:02.2: 13.79 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:02.99 +00:55:57.6: 13.56 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:26:09.21 -04:06:02.2: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:21.46 +01:47:45.5: 13.43 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:09.00 +01:30:04.5: 13.56 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:34.83 +01:24:24.7: 13.72 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:22.93 +00:57:56.6: 13.57 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:57:37.72 -00:00:11.4: 12.90 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:16.31 +01:12:20.5: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:34.83 +01:24:24.7: ref_mag=13.70 +/- 0.04 new_mean_mag=12.3478 delta=1.36 (need > 0.90)
Forced photometry filter KEPT candidate at 20:00:22.93 +00:57:56.6: ref_mag=13.56 +/- 0.03 new_mean_mag=12.4705 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter REJECTED candidate at 19:57:37.72 -00:00:11.4: ref_mag=12.87 +/- 0.02 new_mean_mag=12.0242 delta=0.85 (need > 0.90)
Forced photometry filter KEPT candidate at 19:59:16.31 +01:12:20.5: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1392 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:16.32 +01:07:02.2: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter KEPT candidate at 20:00:16.32 +01:07:02.2: ref_mag=13.77 +/- 0.04 new_mean_mag=12.5989 delta=1.17 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:02.99 +00:55:57.6: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:02.99 +00:55:57.6: ref_mag=13.53 +/- 0.03 new_mean_mag=12.4429 delta=1.09 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:26:09.21 -04:06:02.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 19:26:09.21 -04:06:02.2: ref_mag=13.06 +/- 0.02 new_mean_mag=12.1163 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:21.46 +01:47:45.5: 13.54 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:09.00 +01:30:04.5: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:21.46 +01:47:45.5: ref_mag=13.48 +/- 0.03 new_mean_mag=12.4692 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 20:00:09.00 +01:30:04.5: ref_mag=13.54 +/- 0.03 new_mean_mag=12.3701 delta=1.17 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:30.60 +01:13:50.3: 12.87 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:30.60 +01:13:50.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:30.60 +01:13:50.3: ref_mag=12.85 +/- 0.02 new_mean_mag=11.6333 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:15.30 +01:10:07.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:15.30 +01:10:07.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:15.30 +01:10:07.3: ref_mag=13.44 +/- 0.03 new_mean_mag=12.2380 delta=1.20 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:14.77 +01:04:29.3: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:14.77 +01:04:29.3: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:14.77 +01:04:29.3: ref_mag=13.05 +/- 0.02 new_mean_mag=11.8727 delta=1.18 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:15.11 +01:05:37.4: 13.28 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:53.83 +01:02:57.3: 13.29 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:15.11 +01:05:37.4: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 19:59:15.11 +01:05:37.4: ref_mag=13.32 +/- 0.03 new_mean_mag=12.3116 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.90 +01:40:24.1: 12.83 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:53.83 +01:02:57.3: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter KEPT candidate at 19:58:53.83 +01:02:57.3: ref_mag=13.30 +/- 0.03 new_mean_mag=12.3123 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.90 +01:40:24.1: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:37.90 +01:40:24.1: ref_mag=12.82 +/- 0.02 new_mean_mag=11.7458 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:02.22 +01:10:06.0: 13.10 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:27.76 +00:57:18.9: 12.56 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:02.22 +01:10:06.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:02.22 +01:10:06.0: ref_mag=13.08 +/- 0.02 new_mean_mag=12.1530 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:27.76 +00:57:18.9: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 20:00:27.76 +00:57:18.9: ref_mag=12.60 +/- 0.01 new_mean_mag=11.5956 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:52.17 +00:57:56.4: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:52.17 +00:57:56.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 19:59:52.17 +00:57:56.4: ref_mag=13.28 +/- 0.03 new_mean_mag=12.3315 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:30:37.69 +01:15:00.0: 13.76 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:36.05 +01:02:30.6: 12.54 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:30:37.69 +01:15:00.0: 13.74 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.04 +01:43:48.7: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Forced photometry filter KEPT candidate at 19:30:37.69 +01:15:00.0: ref_mag=13.75 +/- 0.05 new_mean_mag=12.7476 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:36.05 +01:02:30.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 20:00:36.05 +01:02:30.6: ref_mag=12.55 +/- 0.01 new_mean_mag=11.4570 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.04 +01:43:48.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:37.04 +01:43:48.7: ref_mag=12.82 +/- 0.02 new_mean_mag=11.8104 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:29.32 -03:52:42.8: 13.69 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:29.32 -03:52:42.8: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 19:25:29.32 -03:52:42.8: ref_mag=13.65 +/- 0.04 new_mean_mag=12.7253 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.37 +00:54:01.6: 13.24 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.37 +00:54:01.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:37.37 +00:54:01.6: ref_mag=13.28 +/- 0.03 new_mean_mag=12.2650 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:18.84 +01:48:49.9: 13.43 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:38.95 +00:56:00.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:18.84 +01:48:49.9: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:18.84 +01:48:49.9: ref_mag=13.44 +/- 0.03 new_mean_mag=12.3418 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:38.95 +00:56:00.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:38.95 +00:56:00.3: ref_mag=12.79 +/- 0.02 new_mean_mag=11.8598 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:35.50 -03:48:20.0: 13.22 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:35.50 -03:48:20.0: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 19:25:35.50 -03:48:20.0: ref_mag=13.20 +/- 0.03 new_mean_mag=12.2245 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:00.95 +00:57:51.0: 12.46 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:00.95 +00:57:51.0: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter KEPT candidate at 20:00:00.95 +00:57:51.0: ref_mag=12.46 +/- 0.01 new_mean_mag=11.5077 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:38.37 +01:01:10.3: 13.83 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:38.37 +01:01:10.3: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 20:00:38.37 +01:01:10.3: ref_mag=13.78 +/- 0.04 new_mean_mag=12.4230 delta=1.35 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:16.40 +01:03:58.5: 12.74 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:34.56 +00:47:42.2: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:16.40 +01:03:58.5: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:16.40 +01:03:58.5: ref_mag=12.72 +/- 0.02 new_mean_mag=11.7234 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:34.56 +00:47:42.2: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter KEPT candidate at 19:58:34.56 +00:47:42.2: ref_mag=13.52 +/- 0.03 new_mean_mag=12.3915 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:39.29 +01:09:59.8: 12.40 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:39.29 +01:09:59.8: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 20:00:39.29 +01:09:59.8: ref_mag=12.40 +/- 0.01 new_mean_mag=11.1738 delta=1.23 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:17.00 -04:56:56.1: 13.21 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:48.61 +01:14:06.1: 12.39 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:17.00 -04:56:56.1: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 19:25:17.00 -04:56:56.1: ref_mag=13.20 +/- 0.03 new_mean_mag=12.2586 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:48.61 +01:14:06.1: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 19:59:48.61 +01:14:06.1: ref_mag=12.41 +/- 0.01 new_mean_mag=11.4419 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:32.62 +00:45:11.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:32.62 +00:45:11.7: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 19:58:32.62 +00:45:11.7: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0573 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:02.37 +00:55:12.4: 12.97 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:11.41 +01:01:04.7: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:02.37 +00:55:12.4: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:02.37 +00:55:12.4: ref_mag=12.95 +/- 0.02 new_mean_mag=12.0460 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:11.41 +01:01:04.7: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:11.41 +01:01:04.7: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1212 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:46.79 +01:00:03.9: 12.93 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:37.79 +01:08:29.4: 13.36 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:26:17.93 -04:19:09.7: 13.66 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:46.79 +01:00:03.9: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 19:58:46.79 +01:00:03.9: ref_mag=12.95 +/- 0.02 new_mean_mag=12.0108 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:06.38 +00:57:11.0: 12.92 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:37.79 +01:08:29.4: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:37.79 +01:08:29.4: ref_mag=13.36 +/- 0.03 new_mean_mag=12.1162 delta=1.24 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:26:17.93 -04:19:09.7: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry filter KEPT candidate at 19:26:17.93 -04:19:09.7: ref_mag=13.62 +/- 0.04 new_mean_mag=12.5218 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:29.79 +01:11:23.2: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:06.38 +00:57:11.0: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:06.38 +00:57:11.0: ref_mag=12.94 +/- 0.02 new_mean_mag=12.0139 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:29.79 +01:11:23.2: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 19:59:29.79 +01:11:23.2: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1596 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:28.63 +01:46:53.5: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:28.63 +01:46:53.5: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 20:00:28.63 +01:46:53.5: ref_mag=13.47 +/- 0.03 new_mean_mag=12.3823 delta=1.09 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:13.43 +01:02:49.0: 13.38 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:13.43 +01:02:49.0: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 19:59:13.43 +01:02:49.0: ref_mag=13.38 +/- 0.03 new_mean_mag=12.3426 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:59:58.29 +01:15:23.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:59:58.29 +01:15:23.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 19:59:58.29 +01:15:23.6: ref_mag=12.63 +/- 0.01 new_mean_mag=11.5669 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:33.17 +01:07:23.8: 13.12 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:33.17 +01:07:23.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 20:00:33.17 +01:07:23.8: ref_mag=13.11 +/- 0.02 new_mean_mag=11.9623 delta=1.14 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:25:21.42 -03:58:20.5: 13.48 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:25:21.42 -03:58:20.5: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 19:25:21.42 -03:58:20.5: ref_mag=13.42 +/- 0.03 new_mean_mag=12.4901 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 20:00:17.18 +01:16:44.0: 13.76 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-17_03-54-02_20.00sec_4.90C_LIGHT_0389.fits at 19:58:43.21 +00:51:05.3: 13.63 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 20:00:17.18 +01:16:44.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 20:00:17.18 +01:16:44.0: ref_mag=13.73 +/- 0.04 new_mean_mag=12.4094 delta=1.32 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-22_03-33-12_20.00sec_5.00C_LIGHT_0369.fits at 19:58:43.21 +00:51:05.3: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 19:58:43.21 +00:51:05.3: ref_mag=13.60 +/- 0.03 new_mean_mag=12.5103 delta=1.09 (need > 0.90)
Adding exclusion_list_local.txt__out122986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42291.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 78s
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: 28s
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Considering the candidate 185817_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185817_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185819_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185819_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185835_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185835_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185836_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185836_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185837_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185837_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185838_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185838_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185852_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185852_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 185854_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185854_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:25:21.69 -04:07:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185870_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185870_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:28:12.50 +01:29:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185875_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185875_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185876_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185876_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 185877_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185877_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:31:35.88 -05:06:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185879_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 185879_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 190027_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 190027_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:25:07.24 -04:52:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191914_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 191914_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 194547_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 194547_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:26:24.62 +00:19:40.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197621_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 197621_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:59:21.40 +01:20:51.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55210_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 55210_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
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Considering the candidate 31403_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 31403_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 34844_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 34844_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 38680_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 38680_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 36134_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 36134_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 39218_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 39218_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 137621_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 137621_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 29826_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 29826_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 24915_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 24915_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 34397_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 34397_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 35349_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 35349_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 37019_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37019_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 36643_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 36643_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 37358_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37358_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 27032_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 27032_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 35513_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 35513_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 38894_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 38894_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 38681_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 38681_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 33860_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 33860_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 37550_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37550_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 26149_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 26149_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 141284_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 141284_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 39754_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 39754_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 24607_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 24607_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 39351_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 39351_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 141909_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 141909_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 90948_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 90948_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:55:13.48 -02:06:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38833_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 38833_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 37781_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37781_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 37152_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37152_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 41504_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 41504_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
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Considering the candidate 35456_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 35456_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64251_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 64251_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:34:59.67 -00:32:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122986_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 122986_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34346_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 34346_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37683_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 37683_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 20:00:15.18 +01:02:32.0 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56031_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 56031_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:56:17.15 -00:02:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42291_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 42291_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35343_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 35343_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 20:00:28.73 +01:11:10.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39497_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 39497_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37883_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37883_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38190_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 38190_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35820_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 35820_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133832_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 133832_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38953_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 38953_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35038_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 35038_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25172_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 25172_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37705_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 37705_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33983_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 33983_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36148_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 36148_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140047_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 140047_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33457_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 33457_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40535_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
Preparing report for the candidate 40535_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33976_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213
The candidate 33976_fd_Aql-04-Q2b1x1_2026-07-18_01-01-15_20.00sec_4.90C_LIGHT_0213 did not pass the final checks
**** FOUND 19:59:22.59 +01:22:39.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 111s
Prepared the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:00:32.05 +01:38:59.3
20:00:28.72 +01:11:10.4
20:00:15.18 +01:02:31.9
19:25:17.00 -04:56:56.1
19:26:17.93 -04:19:09.7
19:26:09.21 -04:06:02.2
19:25:21.42 -03:58:20.5
19:25:29.32 -03:52:42.8
19:25:35.50 -03:48:20.0
20:00:18.84 +01:48:49.9
20:00:21.46 +01:47:45.5
20:00:28.63 +01:46:53.5
20:00:37.04 +01:43:48.7
20:00:37.90 +01:40:24.1
20:00:09.00 +01:30:04.5
20:00:34.83 +01:24:24.7
20:00:17.18 +01:16:44.0
19:30:37.69 +01:15:00.0
19:59:58.29 +01:15:23.6
19:59:48.61 +01:14:06.1
20:00:30.60 +01:13:50.3
19:59:16.31 +01:12:20.5
19:59:29.79 +01:11:23.2
20:00:15.30 +01:10:07.3
20:00:39.29 +01:09:59.8
20:00:02.22 +01:10:06.0
20:00:37.79 +01:08:29.4
20:00:16.32 +01:07:02.2
20:00:33.17 +01:07:23.8
19:59:15.11 +01:05:37.4
20:00:14.77 +01:04:29.3
20:00:16.40 +01:03:58.5
19:58:53.83 +01:02:57.3
20:00:36.05 +01:02:30.6
19:59:13.43 +01:02:49.0
20:00:38.37 +01:01:10.3
20:00:11.41 +01:01:04.7
19:58:46.79 +01:00:03.9
20:00:22.93 +00:57:56.6
19:59:52.17 +00:57:56.4
20:00:00.95 +00:57:51.0
20:00:27.76 +00:57:18.9
19:59:06.38 +00:57:11.0
20:00:02.99 +00:55:57.6
19:59:38.95 +00:56:00.3
19:59:02.37 +00:55:12.4
20:00:37.37 +00:54:01.6
19:58:43.21 +00:51:05.3
19:58:34.56 +00:47:42.2
19:58:32.62 +00:45:11.7
########### Completed Aql-04-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 ####
20:00:28.72 +01:11:10.4
20:00:32.05 +01:38:59.3
20:00:15.18 +01:02:31.9
20:00:34.83 +01:24:24.7
19:59:16.31 +01:12:20.5
20:00:22.93 +00:57:56.6
20:00:16.32 +01:07:02.2
20:00:02.99 +00:55:57.6
19:26:09.21 -04:06:02.2
20:00:09.00 +01:30:04.5
20:00:21.46 +01:47:45.5
20:00:30.60 +01:13:50.3
20:00:15.30 +01:10:07.3
20:00:14.77 +01:04:29.3
19:59:15.11 +01:05:37.4
19:58:53.83 +01:02:57.3
20:00:37.90 +01:40:24.1
20:00:02.22 +01:10:06.0
20:00:27.76 +00:57:18.9
19:59:52.17 +00:57:56.4
19:30:37.69 +01:15:00.0
20:00:36.05 +01:02:30.6
20:00:37.04 +01:43:48.7
19:25:29.32 -03:52:42.8
20:00:37.37 +00:54:01.6
20:00:18.84 +01:48:49.9
19:59:38.95 +00:56:00.3
19:25:35.50 -03:48:20.0
20:00:00.95 +00:57:51.0
20:00:38.37 +01:01:10.3
20:00:16.40 +01:03:58.5
19:58:34.56 +00:47:42.2
20:00:39.29 +01:09:59.8
19:25:17.00 -04:56:56.1
19:59:48.61 +01:14:06.1
19:58:32.62 +00:45:11.7
19:59:02.37 +00:55:12.4
20:00:11.41 +01:01:04.7
19:58:46.79 +01:00:03.9
20:00:37.79 +01:08:29.4
19:26:17.93 -04:19:09.7
19:59:06.38 +00:57:11.0
19:59:29.79 +01:11:23.2
20:00:28.63 +01:46:53.5
19:59:13.43 +01:02:49.0
19:59:58.29 +01:15:23.6
20:00:33.17 +01:07:23.8
19:25:21.42 -03:58:20.5
20:00:17.18 +01:16:44.0
19:58:43.21 +00:51:05.3
###################################################################################
20:00:28.72 +01:11:10.4 -- not an asteroid (will add it to exclusion list)
20:00:32.05 +01:38:59.3 -- not an asteroid (will add it to exclusion list)
20:00:15.18 +01:02:31.9 -- not an asteroid (will add it to exclusion list)
20:00:34.83 +01:24:24.7 -- not an asteroid (will add it to exclusion list)
19:59:16.31 +01:12:20.5 -- not an asteroid (will add it to exclusion list)
20:00:22.93 +00:57:56.6 -- not an asteroid (will add it to exclusion list)
20:00:16.32 +01:07:02.2 -- not an asteroid (will add it to exclusion list)
20:00:02.99 +00:55:57.6 -- not an asteroid (will add it to exclusion list)
19:26:09.21 -04:06:02.2 -- not an asteroid (will add it to exclusion list)
20:00:09.00 +01:30:04.5 -- not an asteroid (will add it to exclusion list)
20:00:21.46 +01:47:45.5 -- not an asteroid (will add it to exclusion list)
20:00:30.60 +01:13:50.3 -- not an asteroid (will add it to exclusion list)
20:00:15.30 +01:10:07.3 -- not an asteroid (will add it to exclusion list)
20:00:14.77 +01:04:29.3 -- not an asteroid (will add it to exclusion list)
19:59:15.11 +01:05:37.4 -- not an asteroid (will add it to exclusion list)
19:58:53.83 +01:02:57.3 -- not an asteroid (will add it to exclusion list)
20:00:37.90 +01:40:24.1 -- not an asteroid (will add it to exclusion list)
20:00:02.22 +01:10:06.0 -- not an asteroid (will add it to exclusion list)
20:00:27.76 +00:57:18.9 -- not an asteroid (will add it to exclusion list)
19:59:52.17 +00:57:56.4 -- not an asteroid (will add it to exclusion list)
19:30:37.69 +01:15:00.0 -- not an asteroid (will add it to exclusion list)
20:00:36.05 +01:02:30.6 -- not an asteroid (will add it to exclusion list)
20:00:37.04 +01:43:48.7 -- not an asteroid (will add it to exclusion list)
19:25:29.32 -03:52:42.8 -- not an asteroid (will add it to exclusion list)
20:00:37.37 +00:54:01.6 -- not an asteroid (will add it to exclusion list)
20:00:18.84 +01:48:49.9 -- not an asteroid (will add it to exclusion list)
19:59:38.95 +00:56:00.3 -- not an asteroid (will add it to exclusion list)
19:25:35.50 -03:48:20.0 -- not an asteroid (will add it to exclusion list)
20:00:00.95 +00:57:51.0 -- not an asteroid (will add it to exclusion list)
20:00:38.37 +01:01:10.3 -- not an asteroid (will add it to exclusion list)
20:00:16.40 +01:03:58.5 -- not an asteroid (will add it to exclusion list)
19:58:34.56 +00:47:42.2 -- not an asteroid (will add it to exclusion list)
20:00:39.29 +01:09:59.8 -- not an asteroid (will add it to exclusion list)
19:25:17.00 -04:56:56.1 -- not an asteroid (will add it to exclusion list)
19:59:48.61 +01:14:06.1 -- not an asteroid (will add it to exclusion list)
19:58:32.62 +00:45:11.7 -- not an asteroid (will add it to exclusion list)
19:59:02.37 +00:55:12.4 -- not an asteroid (will add it to exclusion list)
20:00:11.41 +01:01:04.7 -- not an asteroid (will add it to exclusion list)
19:58:46.79 +01:00:03.9 -- not an asteroid (will add it to exclusion list)
20:00:37.79 +01:08:29.4 -- not an asteroid (will add it to exclusion list)
19:26:17.93 -04:19:09.7 -- not an asteroid (will add it to exclusion list)
19:59:06.38 +00:57:11.0 -- not an asteroid (will add it to exclusion list)
19:59:29.79 +01:11:23.2 -- not an asteroid (will add it to exclusion list)
20:00:28.63 +01:46:53.5 -- not an asteroid (will add it to exclusion list)
19:59:13.43 +01:02:49.0 -- not an asteroid (will add it to exclusion list)
19:59:58.29 +01:15:23.6 -- not an asteroid (will add it to exclusion list)
20:00:33.17 +01:07:23.8 -- not an asteroid (will add it to exclusion list)
19:25:21.42 -03:58:20.5 -- not an asteroid (will add it to exclusion list)
20:00:17.18 +01:16:44.0 -- not an asteroid (will add it to exclusion list)
19:58:43.21 +00:51:05.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:25:17.00 -04:56:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:21.42 -03:58:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:29.32 -03:52:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:35.50 -03:48:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:09.21 -04:06:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:17.93 -04:19:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:37.69 +01:15:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:32.62 +00:45:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:34.56 +00:47:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:43.21 +00:51:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:46.79 +01:00:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:53.83 +01:02:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:02.37 +00:55:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:06.38 +00:57:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:13.43 +01:02:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:15.11 +01:05:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:16.31 +01:12:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:29.79 +01:11:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:38.95 +00:56:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:48.61 +01:14:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:52.17 +00:57:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:58.29 +01:15:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:00.95 +00:57:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:02.22 +01:10:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:02.99 +00:55:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:09.00 +01:30:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:11.41 +01:01:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:14.77 +01:04:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:15.18 +01:02:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:15.30 +01:10:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:16.32 +01:07:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:16.40 +01:03:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:17.18 +01:16:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:18.84 +01:48:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:21.46 +01:47:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:22.93 +00:57:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:27.76 +00:57:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:28.63 +01:46:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:28.72 +01:11:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:30.60 +01:13:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:32.05 +01:38:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:33.17 +01:07:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:34.83 +01:24:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:36.05 +01:02:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:37.04 +01:43:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:37.37 +00:54:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:37.79 +01:08:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:37.90 +01:40:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:38.37 +01:01:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:39.29 +01:09:59.8 -- 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)
19:25:17.00 -04:56:56.1 -- not a known variable star
19:25:21.42 -03:58:20.5 -- not a known variable star
19:25:29.32 -03:52:42.8 -- not a known variable star
19:25:35.50 -03:48:20.0 -- not a known variable star
19:26:09.21 -04:06:02.2 -- not a known variable star
19:26:17.93 -04:19:09.7 -- not a known variable star
19:30:37.69 +01:15:00.0 -- not a known variable star
19:58:32.62 +00:45:11.7 -- not a known variable star
19:58:34.56 +00:47:42.2 -- not a known variable star
19:58:43.21 +00:51:05.3 -- not a known variable star
19:58:46.79 +01:00:03.9 -- not a known variable star
19:58:53.83 +01:02:57.3 -- not a known variable star
19:59:02.37 +00:55:12.4 -- not a known variable star
19:59:06.38 +00:57:11.0 -- not a known variable star
19:59:13.43 +01:02:49.0 -- not a known variable star
19:59:15.11 +01:05:37.4 -- not a known variable star
19:59:16.31 +01:12:20.5 -- not a known variable star
19:59:29.79 +01:11:23.2 -- not a known variable star
19:59:38.95 +00:56:00.3 -- not a known variable star
19:59:48.61 +01:14:06.1 -- not a known variable star
19:59:52.17 +00:57:56.4 -- not a known variable star
19:59:58.29 +01:15:23.6 -- not a known variable star
20:00:00.95 +00:57:51.0 -- not a known variable star
20:00:02.22 +01:10:06.0 -- not a known variable star
20:00:02.99 +00:55:57.6 -- not a known variable star
20:00:09.00 +01:30:04.5 -- a known variable star
20:00:11.41 +01:01:04.7 -- not a known variable star
20:00:14.77 +01:04:29.3 -- not a known variable star
20:00:15.18 +01:02:31.9 -- not a known variable star
20:00:15.30 +01:10:07.3 -- not a known variable star
20:00:16.32 +01:07:02.2 -- not a known variable star
20:00:16.40 +01:03:58.5 -- not a known variable star
20:00:17.18 +01:16:44.0 -- not a known variable star
20:00:18.84 +01:48:49.9 -- not a known variable star
20:00:21.46 +01:47:45.5 -- not a known variable star
20:00:22.93 +00:57:56.6 -- not a known variable star
20:00:27.76 +00:57:18.9 -- not a known variable star
20:00:28.63 +01:46:53.5 -- not a known variable star
20:00:28.72 +01:11:10.4 -- not a known variable star
20:00:30.60 +01:13:50.3 -- not a known variable star
20:00:32.05 +01:38:59.3 -- not a known variable star
20:00:33.17 +01:07:23.8 -- not a known variable star
20:00:34.83 +01:24:24.7 -- not a known variable star
20:00:36.05 +01:02:30.6 -- not a known variable star
20:00:37.04 +01:43:48.7 -- not a known variable star
20:00:37.37 +00:54:01.6 -- a known variable star
20:00:37.79 +01:08:29.4 -- not a known variable star
20:00:37.90 +01:40:24.1 -- not a known variable star
20:00:38.37 +01:01:10.3 -- not a known variable star
20:00:39.29 +01:09:59.8 -- not a known variable star
Found 48 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
50 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 50 (excluding asteroids and hot pixels, 48 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461239.75033411 -observatory V36
07:12:35.92 +17:30:49.0 Mercury (4.0mag)
10:44:00.29 +09:06:08.0 Venus (-4.2mag)
04:47:35.25 +22:18:12.8 Mars (1.3mag)
08:23:52.27 +19:48:15.4 Jupiter (-1.8mag)
00:56:31.52 +03:22:19.6 Saturn (0.7mag)
04:08:40.71 +20:48:55.9 Uranus (5.8mag)
00:16:55.66 +00:19:36.5 Neptune (7.7mag)
20:30:10.45 -23:21:28.8 Pluto (14.4mag)
11:06:19.39 +03:14:30.2 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jul 18 04:14 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461239.75033411:
08:23:49.44 +19:48:26.0 Io (6.0mag)
08:24:03.63 +19:47:31.8 Europa (6.3mag)
08:24:08.61 +19:47:11.0 Ganymede (5.6mag)
08:23:26.16 +19:49:56.5 Callisto (6.8mag)
08:22:03.11 +19:35:57.9 Himalia (15.7mag)
08:23:51.73 +19:48:18.5 Thebe (16.6mag)
08:21:24.13 +19:38:42.2 Elara (17.7mag)
08:27:38.03 +19:38:13.5 Pasiphae (17.9mag)
08:28:22.52 +19:54:32.3 Carme (19.0mag)
00:56:41.84 +03:22:26.8 Titan (8.5mag)
00:56:31.36 +03:22:29.7 Rhea (9.8mag)
00:55:57.02 +03:20:10.3 Iapetus (11.2mag)
00:56:18.37 +03:22:10.9 Hyperion (14.5mag)
00:56:21.68 +03:18:24.6 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 04:14 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.75033411:
17:58:56.45 -31:05:44.8 JWST
16:11:03.06 +50:14:43.3 Chandra
21:35:55.44 +50:06:41.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 04:14 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.75033411 -observatory V36
02:47:18.02 +15:20:16.6 17.8mag P/1996 R2 (Lagerkvist)
18:12:10.14 -34:32:34.6 13.8mag P/2010 H2 (Vales)
06:33:33.11 -68:17:05.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:30.07 +32:35:04.2 17.6mag C/2017 K2 (PANSTARRS)
02:28:04.97 +21:13:40.1 15.8mag P/2021 N1 (ZTF)
22:54:31.65 +32:13:30.4 17.3mag C/2022 E2 (ATLAS)
06:21:18.81 +26:50:49.8 16.7mag C/2022 N2 (PANSTARRS)
10:02:27.97 +29:25:29.8 16.9mag C/2022 QE78 (ATLAS)
09:14:52.61 +05:07:58.3 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.77 -11:35:04.5 17.8mag P/2023 B1 (PANSTARRS)
21:39:18.01 +67:29:05.8 17.9mag C/2023 H5 (Lemmon)
16:16:13.46 -10:53:41.1 14.0mag C/2023 R1 (PANSTARRS)
08:14:35.14 +66:08:53.3 17.9mag C/2024 A1 (ATLAS)
07:43:00.65 +30:23:37.0 14.8mag C/2024 E1 (Wierzchos)
15:12:48.73 +15:30:00.8 17.6mag C/2024 G6 (ATLAS)
19:31:01.21 +40:48:43.6 13.7mag C/2024 J3 (ATLAS)
21:38:54.51 +47:07:47.7 17.8mag C/2024 R4 (PANSTARRS)
04:57:00.41 -13:28:10.7 15.7mag C/2024 T5 (ATLAS)
06:40:59.75 +27:44:58.2 18.0mag C/2025 J1 (Borisov)
07:19:38.78 -13:37:59.3 16.9mag C/2025 R3 (PANSTARRS)
10:05:28.45 +22:04:43.7 17.5mag C/2025 V2 (Rankin)
12:47:31.14 +03:34:32.3 17.0mag C/2025 Y1 (ATLAS)
16:31:06.12 +79:07:47.3 17.2mag C/2026 A2 (Bok)
02:54:05.63 +45:33:52.5 16.8mag C/2026 B2 (Sun-Gao)
11:30:45.26 +05:51:44.5 17.0mag A/2026 E1
21:31:07.44 -18:06:29.6 7.1mag 10P/Tempel
11:17:17.92 -02:14:37.5 16.2mag 29P/Schwassmann-Wachmann
04:11:25.85 +30:23:45.1 17.9mag 47P/Ashbrook-Jackson
10:24:32.33 +11:28:46.0 17.1mag 63P/Wild
00:51:23.19 -05:02:47.7 15.5mag 65P/Gunn
04:46:26.11 +20:31:32.7 13.7mag 78P/Gehrels
02:34:38.62 +11:38:33.6 16.4mag 88P/Howell
06:58:44.46 +29:59:05.3 15.8mag 93P/Lovas
04:46:50.11 +31:19:48.3 16.7mag 114P/Wiseman-Skiff
08:27:58.98 +29:46:08.3 15.2mag 123P/West-Hartley
11:02:58.12 -02:00:41.6 16.9mag 124P/Mrkos
05:04:21.04 +21:00:35.8 16.2mag 128P/Shoemaker-Holt
05:51:02.81 +19:36:49.0 17.8mag 131P/Mueller
07:41:40.01 +15:15:44.5 16.5mag 141P-D/Machholz
03:20:17.72 -20:45:08.0 15.1mag 161P/Hartley-IRAS
06:01:34.15 +35:29:36.0 15.5mag 162P/SidingSpring
18:39:23.64 +20:29:50.0 14.0mag 169P/NEAT
01:59:32.09 +08:24:21.2 17.6mag 220P/McNaught
16:35:32.54 -08:44:34.0 17.2mag 235P/LINEAR
09:01:48.18 +32:32:37.1 18.0mag 240P/NEAT
20:37:57.90 -51:08:25.9 17.8mag 259P/Garradd
02:21:33.82 +15:46:58.3 15.6mag 260P/McNaught
06:01:17.84 +37:23:06.6 17.3mag 295P/LINEAR
15:06:33.39 +05:19:36.5 17.6mag 391P/Kowalski
08:41:44.03 +19:20:49.9 17.9mag 450P/LONEOS
08:04:05.95 +38:33:13.6 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 04:14 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
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
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
-rw-r--r-- 1 apache apache 5.6K Jul 18 04:14 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 18 04:14 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:35:24.753 -14:51:35.01 AT 2026svz 2026-06-27.33 22.2271
20:31:55.032 -25:17:26.05 AT 2026svy 2026-06-27.32 22.425
23:12:03.386 -07:08:51.16 AT 2026svx 2026-06-27.43 22.3341
21:38:52.469 -09:12:08.16 AT 2026svw 2026-06-27.33 20.826
21:24:07.399 -08:10:48.32 AT 2026svv 2026-06-27.34 22.9964
20:42:22.608 -20:56:09.99 AT 2026svu 2026-06-27.32 22.8033
22:49:29.419 -09:52:21.90 AT 2026svt 2026-06-27.41 23.2399
23:08:56.975 -10:56:50.31 AT 2026svs 2026-06-27.42 23.0562
23:03:48.038 -10:42:20.17 AT 2026svr 2026-06-27.42 23.1156
21:05:20.116 -12:39:02.09 AT 2026svq 2026-06-27.30 22.4649
04:03:37.997 -49:14:19.96 AT 2026svp 2026-06-26.43 23.1019
21:42:26.450 -12:30:39.78 AT 2026svo 2026-06-26.41 23.1202
22:23:57.549 -05:26:28.43 AT 2026svn 2026-06-26.40 23.0846
21:59:30.646 -08:36:23.43 AT 2026svm 2026-06-26.41 23.0458
00:40:45.913 -42:36:08.06 AT 2026svl 2026-06-26.42 23.627
22:01:49.708 -02:28:35.92 AT 2026svk 2026-06-26.41 22.3804
22:26:37.642 -04:12:59.57 AT 2026svj 2026-06-26.40 22.8575
21:46:45.471 -13:57:34.56 AT 2026svi 2026-06-26.41 22.7499
21:42:08.217 -14:29:27.43 AT 2026svh 2026-06-26.41 23.2705
21:57:43.950 -02:48:28.98 AT 2026svg 2026-06-26.41 21.5213
-rw-r--r-- 1 apache apache 89K Jul 18 04:14 tns_transients_list.txt
