This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB
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 18.2673 2461239.7673 12.28 20:36:36.83 +00:16:14.5
45.88423 -23.08433 galactic Aql Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:36:36.83 +00:16:14.5 (user input) | T | P | (position from user input) J-Ks=0.937+/-0.030 (M)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:36:36.83 +00:16:14.5: 13.32 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:36:36.83 +00:16:14.5: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 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,2461239.7673,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.38 20:16:06.46 -02:56:32.1
40.19871 -20.14222 galactic Aql Second-epoch detections are separated by 0.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.0290-02.9401 | 20:16:06.46 -02:56:32.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.346+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:06.46 -02:56:32.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:06.46 -02:56:32.1: 13.39 +/- 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 J304.0290-02.9401,2461239.7673,12.38,0.05,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 J304.0290-02.9401 20260718.2673 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 18.2673 2461239.7673 12.28 20:16:20.76 -02:29:11.0
40.65712 -19.98115 galactic Aql Second-epoch detections are separated by 2.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:20.76 -02:29:11.0 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.032 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:20.76 -02:29:11.0: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:20.76 -02:29:11.0: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461239.7673,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.10 20:16:31.57 -02:48:05.6
40.38325 -20.16874 galactic Aql Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4222615174584200576 | 20:16:30.82 -02:48:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.749+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:31.57 -02:48:05.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:31.57 -02:48:05.6: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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 4222615174584200576,2461239.7673,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4222615174584200576 20260718.2673 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.59 20:36:48.45 +00:16:39.5
45.91698 -23.12286 galactic Aql Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.2008+00.2840 | 20:36:48.45 +00:16:39.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.384+/-0.032 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:36:48.45 +00:16:39.5: 13.67 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:36:48.45 +00:16:39.5: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 J309.2008+00.2840,2461239.7673,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.2008+00.2840 20260718.2673 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.30 20:23:46.13 -04:11:11.4
39.97319 -22.41335 galactic Aql Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:46.13 -04:11:11.4 (user input) | T | P | (position from user input) J-Ks=0.333+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:46.13 -04:11:11.4: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:46.13 -04:11:11.4: 13.50 +/- 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
target,2461239.7673,12.30,0.05,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 20260718.2673 12.30CV 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 18.2673 2461239.7673 12.12 20:37:38.50 +00:00:54.3
45.78198 -23.43438 galactic Aql Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:37:38.50 +00:00:54.3 (user input) | T | P | (position from user input) J-Ks=0.578+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:38.50 +00:00:54.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:38.50 +00:00:54.3: 13.16 +/- 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,2461239.7673,12.12,0.05,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 20260718.2673 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.42 20:43:36.06 -00:01:45.2
46.55505 -24.74722 galactic Aqr Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4227987865134432512 | 20:43:35.45 -00:01:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.597+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:43:36.06 -00:01:45.2: 13.52 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:43:36.06 -00:01:45.2: 13.44 +/- 0.04 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
Gaia DR3 4227987865134432512,2461239.7673,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4227987865134432512 20260718.2673 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.71 20:39:57.41 +00:21:22.6
46.41983 -23.76569 galactic Aqr Second-epoch detections are separated by 0.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.9880+00.3595 | 20:39:57.41 +00:21:22.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.543+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:39:57.41 +00:21:22.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:39:57.41 +00:21:22.6: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 J309.9880+00.3595,2461239.7673,12.71,0.05,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
ATO J309.9880+00.3595 20260718.2673 12.71CV 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 18.2673 2461239.7673 11.21 20:37:19.38 +00:10:11.5
45.88508 -23.28829 galactic Aql Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4231137313114275072 | 20:37:19.33 +00:10:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:19.38 +00:10:11.5: 12.19 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:19.38 +00:10:11.5: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4231137313114275072,2461239.7673,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4231137313114275072 20260718.2673 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 18.2673 2461239.7673 12.02 20:15:52.15 -02:15:14.8
40.81552 -19.76679 galactic Aql Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9669-02.2448 | 20:15:52.15 -02:15:14.8 (user input) | PULSE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.599+/-0.031 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:52.15 -02:15:14.8: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:52.15 -02:15:14.8: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 J303.9669-02.2448,2461239.7673,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.9669-02.2448 20260718.2673 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.29 20:15:29.40 -03:06:16.4
39.96919 -20.08165 galactic Aql Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8797-03.1035 | 20:15:29.37 -03:06:16.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.954+/-0.033 (M)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:29.40 -03:06:16.4: 12.20 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:29.40 -03:06:16.4: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 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 J303.8797-03.1035,2461239.7673,11.29,0.05,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
ATO J303.8797-03.1035 20260718.2673 11.29CV 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 18.2673 2461239.7673 10.79 20:24:11.19 -04:12:05.7
40.01107 -22.51258 galactic Aql Second-epoch detections are separated by 0.5" and 6.6 pix
The object was found in VSX23" Gaia DR3 4219399751608760064
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
19.900 G 20.080 G
ATTENTION: measured mag 10.79 is 9.1 mag brighter than the VSX record maximum brightness 19.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:24:11.19 -04:12:05.7: 11.70 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:24:11.19 -04:12:05.7: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 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 4219399751608760064,2461239.7673,10.79,0.05,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 4219399751608760064 20260718.2673 10.79CV 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 18.2673 2461239.7673 10.80 20:15:54.83 -02:17:07.2
40.79182 -19.79134 galactic Aql Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9784-02.2852 | 20:15:54.82 -02:17:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.693+/-0.031 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:54.83 -02:17:07.2: 11.76 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:54.83 -02:17:07.2: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.9784-02.2852,2461239.7673,10.80,0.05,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 J303.9784-02.2852 20260718.2673 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.20 20:15:01.73 -03:07:21.6
39.89500 -19.98825 galactic Aql Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.25218 1998 TZ1 -180 521 551 17.4 -0 -0
ATTENTION: measured mag 12.20 is 5.2 mag brighter than the predicted asteroid brightness 17.4 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:01.73 -03:07:21.6: 13.21 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:01.73 -03:07:21.6: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.7673,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260718.2673 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.14 20:23:56.65 -04:09:32.4
40.02150 -22.43929 galactic Aql Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:56.65 -04:09:32.4 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.036 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:56.65 -04:09:32.4: 13.23 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:56.65 -04:09:32.4: 13.13 +/- 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,2461239.7673,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.39 20:15:33.59 -02:06:17.0
40.91682 -19.62826 galactic Aql Second-epoch detections are separated by 1.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:33.59 -02:06:17.0 (user input) | T | P | (position from user input) J-Ks=0.679+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:33.59 -02:06:17.0: 13.43 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:33.59 -02:06:17.0: 13.45 +/- 0.05 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,2461239.7673,12.39,0.05,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 20260718.2673 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 18.2673 2461239.7673 11.88 20:15:46.96 -02:21:54.7
40.70054 -19.79999 galactic Aql Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9454-02.3653 | 20:15:46.96 -02:21:54.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.307+/-0.032 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:46.96 -02:21:54.7: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:46.96 -02:21:54.7: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J303.9454-02.3653,2461239.7673,11.88,0.05,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 J303.9454-02.3653 20260718.2673 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 18.2673 2461239.7673 12.57 20:15:42.25 -02:50:35.1
40.24188 -20.00680 galactic Aql Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:42.25 -02:50:35.1 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.033 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:42.25 -02:50:35.1: 13.78 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:42.25 -02:50:35.1: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461239.7673,12.57,0.05,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
target 20260718.2673 12.57CV 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 18.2673 2461239.7673 12.23 20:37:37.61 +00:00:28.4
45.77316 -23.43474 galactic Aql Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:37:37.61 +00:00:28.4 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.033 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:37.61 +00:00:28.4: 13.26 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:37.61 +00:00:28.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,12.23,0.05,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 20260718.2673 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.18 20:16:11.07 -02:44:06.9
40.40307 -20.06230 galactic Aql Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:11.07 -02:44:06.9 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.032 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:11.07 -02:44:06.9: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:11.07 -02:44:06.9: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461239.7673,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.99 20:15:57.81 -02:22:40.1
40.71129 -19.84578 galactic Aql Second-epoch detections are separated by 0.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:57.81 -02:22:40.1 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.032 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:57.81 -02:22:40.1: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:57.81 -02:22:40.1: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461239.7673,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.74 20:37:35.57 -00:01:18.0
45.74061 -23.44205 galactic Aql Second-epoch detections are separated by 0.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:37:35.57 -00:01:18.0 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.031 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:35.57 -00:01:18.0: 13.80 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:35.57 -00:01:18.0: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461239.7673,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.71 20:38:07.64 +00:19:55.7
46.14745 -23.38171 galactic Aql Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:38:07.64 +00:19:55.7 (user input) | T | P | (position from user input) J-Ks=0.801+/-0.034 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:38:07.64 +00:19:55.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:38:07.64 +00:19:55.7: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461239.7673,12.71,0.05,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 20260718.2673 12.71CV 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 18.2673 2461239.7673 11.92 20:23:30.57 -04:14:23.9
39.88950 -22.38090 galactic Aql Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.8772-04.2400 | 20:23:30.57 -04:14:23.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.691+/-0.035 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:30.57 -04:14:23.9: 12.81 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:30.57 -04:14:23.9: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J305.8772-04.2400,2461239.7673,11.92,0.05,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 J305.8772-04.2400 20260718.2673 11.92CV 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 18.2673 2461239.7673 12.63 20:38:48.40 +00:18:30.8
46.21766 -23.54061 galactic Aqr Second-epoch detections are separated by 0.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:38:48.40 +00:18:30.8 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.035 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:38:48.40 +00:18:30.8: 13.79 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:38:48.40 +00:18:30.8: 13.76 +/- 0.05 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,2461239.7673,12.63,0.05,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 20260718.2673 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 18.2673 2461239.7673 12.49 20:15:31.14 -02:21:26.8
40.67491 -19.73822 galactic Aql Second-epoch detections are separated by 1.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8783-02.3598 | 20:15:31.14 -02:21:26.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.390+/-0.033 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:31.14 -02:21:26.8: 13.65 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:31.14 -02:21:26.8: 13.65 +/- 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
ATO J303.8783-02.3598,2461239.7673,12.49,0.05,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 J303.8783-02.3598 20260718.2673 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.27 20:15:06.12 -02:36:09.6
40.39290 -19.76136 galactic Aql Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin -392 18 392 16.2 -0 -0
ATTENTION: measured mag 12.27 is 3.9 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:06.12 -02:36:09.6: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:06.12 -02:36:09.6: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
VARIABLE_NAME,2461239.7673,12.27,0.05,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
VARIABLE_NAME 20260718.2673 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 18.2673 2461239.7673 12.16 20:15:36.95 -02:13:04.3
40.81784 -19.69390 galactic Aql Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:36.95 -02:13:04.3 (user input) | T | P | (position from user input) J-Ks=0.801+/-0.029 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:36.95 -02:13:04.3: 13.25 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:36.95 -02:13:04.3: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,12.16,0.05,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 20260718.2673 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 18.2673 2461239.7673 12.36 20:13:58.83 -03:12:40.4
39.68208 -19.79790 galactic Aql Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.992 Swasey 300 425 520 15.0 -0 -0
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:13:58.83 -03:12:40.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:13:58.83 -03:12:40.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.7673,12.36,0.05,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
VARIABLE_NAME 20260718.2673 12.36CV 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 18.2673 2461239.7673 12.90 20:37:19.37 +00:00:11.1
45.72747 -23.37118 galactic Aql Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.3260+00.0120 | 20:37:19.37 +00:00:11.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M3 2008AJ....135..785W SDSS J203720.20+000030.3 J-Ks=0.640+/-0.034 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:19.37 +00:00:11.1: 14.15 +/- 0.07 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:19.37 +00:00:11.1: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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
ATO J309.3260+00.0120,2461239.7673,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.3260+00.0120 20260718.2673 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.87 20:16:03.62 -02:36:58.2
40.49955 -19.97908 galactic Aql Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin 470 -31 471 16.2 -0 -0
ATTENTION: measured mag 11.87 is 4.3 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:03.62 -02:36:58.2: 12.80 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:03.62 -02:36:58.2: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.7673,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260718.2673 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.23 20:16:05.66 -02:28:02.1
40.64367 -19.91667 galactic Aql Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:05.66 -02:28:02.1 (user input) | T | P | (position from user input) J-Ks=0.928+/-0.030 (M)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:05.66 -02:28:02.1: 13.43 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:05.66 -02:28:02.1: 13.35 +/- 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
target,2461239.7673,12.23,0.05,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 20260718.2673 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.11 20:16:05.93 -02:56:55.1
40.19160 -20.14326 galactic Aql Second-epoch detections are separated by 2.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.0290-02.9401 | 20:16:05.93 -02:56:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.469+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:05.93 -02:56:55.1: 13.06 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:05.93 -02:56:55.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 J304.0290-02.9401,2461239.7673,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.0290-02.9401 20260718.2673 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.09 20:14:43.14 -02:36:01.6
40.34738 -19.67582 galactic Aql Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.6762-02.6028 | 20:14:43.14 -02:36:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.484+/-0.032 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:43.14 -02:36:01.6: 13.07 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:43.14 -02:36:01.6: 13.03 +/- 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 J303.6762-02.6028,2461239.7673,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.6762-02.6028 20260718.2673 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.51 20:14:21.22 -01:57:46.7
40.89875 -19.29567 galactic Aql Second-epoch detections are separated by 0.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.5842-01.9622 | 20:14:21.19 -01:57:46.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.722+/-0.029 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:21.22 -01:57:46.7: 12.41 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:21.22 -01:57:46.7: 12.51 +/- 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
ATO J303.5842-01.9622,2461239.7673,11.51,0.05,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
ATO J303.5842-01.9622 20260718.2673 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 18.2673 2461239.7673 11.89 20:23:48.53 -04:14:03.1
39.93250 -22.44433 galactic Aql Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:48.53 -04:14:03.1 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:48.53 -04:14:03.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:48.53 -04:14:03.1: 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
target,2461239.7673,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.04 20:23:39.55 -04:14:24.3
39.90812 -22.41401 galactic Aql Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:39.55 -04:14:24.3 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.033 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:39.55 -04:14:24.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:39.55 -04:14:24.3: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 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 18.2673 2461239.7673 12.29 20:15:20.88 -02:48:06.9
40.23633 -19.90894 galactic Aql Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:20.88 -02:48:06.9 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.034 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:20.88 -02:48:06.9: 13.25 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:20.88 -02:48:06.9: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461239.7673,12.29,0.05,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 20260718.2673 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 18.2673 2461239.7673 12.15 20:15:44.99 -02:44:46.7
40.33856 -19.97158 galactic Aql Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin 190 -500 535 16.2 -0 -0
ATTENTION: measured mag 12.15 is 4.0 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:44.99 -02:44:46.7: 13.23 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:44.99 -02:44:46.7: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 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
VARIABLE_NAME,2461239.7673,12.15,0.05,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
VARIABLE_NAME 20260718.2673 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 18.2673 2461239.7673 11.86 20:15:32.14 -02:58:22.3
40.09884 -20.03027 galactic Aql Second-epoch detections are separated by 1.7" and 6.4 pix
The object was found in VSX 1" V0587 Aql
Type: SRB
# Max. Min./Amp. JD0 Period
12.300 V 13.800 V 2452473.90000 167.380035000000 M5-M7
The object was not found in astcheck.
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:32.14 -02:58:22.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:32.14 -02:58:22.3: 13.06 +/- 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
V0587 Aql,2461239.7673,11.86,0.05,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
V0587 Aql 20260718.2673 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 18.2673 2461239.7673 11.54 20:15:54.39 -02:22:34.8
40.70555 -19.83253 galactic Aql Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223060751670851328 | 20:15:54.36 -02:22:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.978+/-0.031 (M)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:54.39 -02:22:34.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:54.39 -02:22:34.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 4223060751670851328,2461239.7673,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4223060751670851328 20260718.2673 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.32 20:15:54.16 -02:12:26.6
40.86350 -19.75218 galactic Aql Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9740-02.2068 | 20:15:54.16 -02:12:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.722+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:54.16 -02:12:26.6: 13.41 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:54.16 -02:12:26.6: 13.43 +/- 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 J303.9740-02.2068,2461239.7673,12.32,0.05,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 J303.9740-02.2068 20260718.2673 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 18.2673 2461239.7673 12.29 20:15:22.65 -02:26:19.2
40.58109 -19.74518 galactic Aql Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:22.65 -02:26:19.2 (user input) | T | P | (position from user input) J-Ks=0.769+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:22.65 -02:26:19.2: 13.42 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:22.65 -02:26:19.2: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461239.7673,12.29,0.05,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 20260718.2673 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 18.2673 2461239.7673 11.74 20:15:28.95 -02:25:48.0
40.60231 -19.76426 galactic Aql Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223061610663738752 | 20:15:28.96 -02:25:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.680+/-0.030 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:28.95 -02:25:48.0: 12.74 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:28.95 -02:25:48.0: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 4223061610663738752,2461239.7673,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4223061610663738752 20260718.2673 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.19 20:16:03.80 -02:20:06.7
40.76374 -19.84775 galactic Aql Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:03.80 -02:20:06.7 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.031 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:03.80 -02:20:06.7: 13.38 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:03.80 -02:20:06.7: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461239.7673,12.19,0.05,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 20260718.2673 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 18.2673 2461239.7673 12.18 20:15:32.62 -02:56:38.8
40.12689 -20.01860 galactic Aql Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:32.62 -02:56:38.8 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:32.62 -02:56:38.8: 13.23 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:32.62 -02:56:38.8: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 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,2461239.7673,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.02 20:15:24.24 -02:21:57.1
40.65267 -19.71682 galactic Aql Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:24.24 -02:21:57.1 (user input) | T | P | (position from user input) J-Ks=0.454+/-0.034 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:24.24 -02:21:57.1: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:24.24 -02:21:57.1: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.26 20:16:21.09 -02:54:29.5
40.26111 -20.18011 galactic Aql Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:21.09 -02:54:29.5 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.037 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:21.09 -02:54:29.5: 13.24 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:21.09 -02:54:29.5: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461239.7673,12.26,0.05,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 20260718.2673 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.69 20:15:51.41 -02:27:26.6
40.62329 -19.85967 galactic Aql Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9644-02.4542 | 20:15:51.41 -02:27:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.246+/-0.032 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:51.41 -02:27:26.6: 12.70 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:51.41 -02:27:26.6: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.9644-02.4542,2461239.7673,11.69,0.05,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 J303.9644-02.4542 20260718.2673 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.13 20:15:24.74 -02:50:50.2
40.20167 -19.94435 galactic Aql Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8529-02.8473 | 20:15:24.74 -02:50:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.691+/-0.030 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:24.74 -02:50:50.2: 13.20 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:24.74 -02:50:50.2: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 J303.8529-02.8473,2461239.7673,12.13,0.05,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
ATO J303.8529-02.8473 20260718.2673 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 18.2673 2461239.7673 11.44 20:14:16.12 -03:11:57.0
39.72900 -19.85596 galactic Aql Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.5670-03.1990 | 20:14:16.10 -03:11:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.030 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:16.12 -03:11:57.0: 12.32 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:16.12 -03:11:57.0: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 J303.5670-03.1990,2461239.7673,11.44,0.05,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
ATO J303.5670-03.1990 20260718.2673 11.44CV 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 18.2673 2461239.7673 12.55 20:37:26.59 +00:07:23.6
45.85730 -23.33755 galactic Aql Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:37:26.59 +00:07:23.6 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:26.59 +00:07:23.6: 13.73 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:26.59 +00:07:23.6: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 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,2461239.7673,12.55,0.05,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 20260718.2673 12.55CV 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 18.2673 2461239.7673 12.49 20:15:28.25 -02:21:20.0
40.67067 -19.72671 galactic Aql Second-epoch detections are separated by 2.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8783-02.3598 | 20:15:28.25 -02:21:20.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.409+/-0.034 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:28.25 -02:21:20.0: 13.73 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:28.25 -02:21:20.0: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 J303.8783-02.3598,2461239.7673,12.49,0.05,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 J303.8783-02.3598 20260718.2673 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.03 20:14:52.21 -03:10:30.0
39.82609 -19.97759 galactic Aql Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.25218 1998 TZ1 -323 333 464 17.4 -0 -0
ATTENTION: measured mag 12.03 is 5.4 mag brighter than the predicted asteroid brightness 17.4 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:52.21 -03:10:30.0: 12.94 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:52.21 -03:10:30.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.7673,12.03,0.05,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
VARIABLE_NAME 20260718.2673 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 18.2673 2461239.7673 11.41 20:15:04.32 -02:26:07.7
40.54603 -19.67631 galactic Aql Second-epoch detections are separated by 0.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4222687192595655424 | 20:15:04.31 -02:26:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.861+/-0.033 (M)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:04.32 -02:26:07.7: 12.30 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:04.32 -02:26:07.7: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 4222687192595655424,2461239.7673,11.41,0.05,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 4222687192595655424 20260718.2673 11.41CV 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 18.2673 2461239.7673 11.36 20:23:56.24 -04:17:37.3
39.89155 -22.50031 galactic Aql Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.9893-04.2964 | 20:23:56.21 -04:17:37.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.377+/-0.030 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:56.24 -04:17:37.3: 12.29 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:56.24 -04:17:37.3: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 J305.9893-04.2964,2461239.7673,11.36,0.05,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 J305.9893-04.2964 20260718.2673 11.36CV 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 18.2673 2461239.7673 11.52 20:14:34.94 -03:07:41.5
39.83455 -19.89221 galactic Aql Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.6433-03.1309 | 20:14:34.94 -03:07:41.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.607+/-0.039 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:34.94 -03:07:41.5: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:34.94 -03:07:41.5: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 J303.6433-03.1309,2461239.7673,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.6433-03.1309 20260718.2673 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 10.72 20:15:59.41 -02:20:20.6
40.75097 -19.83344 galactic Aql Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223061267068377728 | 20:15:59.41 -02:20:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.031 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:59.41 -02:20:20.6: 11.75 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:59.41 -02:20:20.6: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 4223061267068377728,2461239.7673,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4223061267068377728 20260718.2673 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.29 20:15:48.69 -02:12:45.0
40.84731 -19.73449 galactic Aql Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9586-02.2239 | 20:15:50.06 -02:13:26.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.031 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:48.69 -02:12:45.0: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:48.69 -02:12:45.0: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.9586-02.2239,2461239.7673,11.29,0.05,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
ATO J303.9586-02.2239 20260718.2673 11.29CV 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 18.2673 2461239.7673 11.77 20:15:08.67 -02:05:03.4
40.88406 -19.52711 galactic Aql Second-epoch detections are separated by 0.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223828103410664448 | 20:15:08.64 -02:05:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.351+/-0.033 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:08.67 -02:05:03.4: 12.67 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:08.67 -02:05:03.4: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4223828103410664448,2461239.7673,11.77,0.05,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 4223828103410664448 20260718.2673 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.46 20:14:17.31 -03:10:38.9
39.75186 -19.85025 galactic Aql Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4222572804729543808 | 20:14:17.31 -03:10:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.031 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:17.31 -03:10:38.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:17.31 -03:10:38.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 4222572804729543808,2461239.7673,11.46,0.05,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 4222572804729543808 20260718.2673 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 18.2673 2461239.7673 12.11 20:15:11.65 -02:14:55.3
40.73631 -19.61547 galactic Aql Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:11.65 -02:14:55.3 (user input) | T | P | (position from user input) J-Ks=0.245+/-0.035 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:11.65 -02:14:55.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:11.65 -02:14:55.3: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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,2461239.7673,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.23 20:15:30.95 -02:42:46.9
40.34073 -19.90436 galactic Aql Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin -20 -380 380 16.2 -0 -0
ATTENTION: measured mag 12.23 is 4.0 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:30.95 -02:42:46.9: 13.18 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:30.95 -02:42:46.9: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 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
VARIABLE_NAME,2461239.7673,12.23,0.05,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
VARIABLE_NAME 20260718.2673 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.88 20:14:59.73 -03:05:25.5
39.92123 -19.96585 galactic Aql Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:59.73 -03:05:25.5 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.032 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:59.73 -03:05:25.5: 12.93 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:59.73 -03:05:25.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,11.88,0.05,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 20260718.2673 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 18.2673 2461239.7673 11.94 20:15:23.51 -02:25:46.8
40.59132 -19.74411 galactic Aql Second-epoch detections are separated by 1.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:23.51 -02:25:46.8 (user input) | T | P | (position from user input) J-Ks=0.464+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:23.51 -02:25:46.8: 12.94 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:23.51 -02:25:46.8: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,11.94,0.05,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 20260718.2673 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.62 20:16:07.67 -02:50:01.0
40.30348 -20.09586 galactic Aql Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:07.67 -02:50:01.0 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:07.67 -02:50:01.0: 13.70 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:07.67 -02:50:01.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461239.7673,12.62,0.05,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 20260718.2673 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 18.2673 2461239.7673 12.18 20:15:40.01 -02:56:51.0
40.13900 -20.04737 galactic Aql Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:40.01 -02:56:51.0 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:40.01 -02:56:51.0: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:40.01 -02:56:51.0: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7673,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.17 20:15:29.25 -03:03:15.6
40.01617 -20.05767 galactic Aql Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:29.25 -03:03:15.6 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.035 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:29.25 -03:03:15.6: 13.18 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:29.25 -03:03:15.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 10.71 20:15:43.53 -02:27:24.4
40.60748 -19.83042 galactic Aql Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin 169 543 568 16.2 -0 -0
ATTENTION: measured mag 10.71 is 5.5 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:43.53 -02:27:24.4: 11.60 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:43.53 -02:27:24.4: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 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
VARIABLE_NAME,2461239.7673,10.71,0.05,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
VARIABLE_NAME 20260718.2673 10.71CV 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 18.2673 2461239.7673 11.65 20:13:59.50 -01:57:29.9
40.85796 -19.21370 galactic Aql Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223886514966121088 | 20:13:57.66 -01:57:39.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.033 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:13:59.50 -01:57:29.9: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:13:59.50 -01:57:29.9: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 4223886514966121088,2461239.7673,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4223886514966121088 20260718.2673 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.38 20:14:13.24 -01:54:59.0
40.92568 -19.24440 galactic Aql Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.5534-01.9206 | 20:14:13.20 -01:54:59.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.377+/-0.029 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:13.24 -01:54:59.0: 12.19 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:13.24 -01:54:59.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J303.5534-01.9206,2461239.7673,11.38,0.05,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 J303.5534-01.9206 20260718.2673 11.38CV 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 18.2673 2461239.7673 11.32 20:15:02.84 -02:33:54.1
40.42143 -19.73165 galactic Aql Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin -441 153 467 16.2 -0 -0
ATTENTION: measured mag 11.32 is 4.9 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:02.84 -02:33:54.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:02.84 -02:33:54.1: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.7673,11.32,0.05,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
VARIABLE_NAME 20260718.2673 11.32CV 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 18.2673 2461239.7673 11.75 20:15:09.85 -02:42:23.3
40.30316 -19.82370 galactic Aql Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin -336 -356 490 16.2 -0 -0
ATTENTION: measured mag 11.75 is 4.4 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:09.85 -02:42:23.3: 12.63 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:09.85 -02:42:23.3: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461239.7673,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260718.2673 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 10.68 20:15:41.35 -02:23:51.8
40.65836 -19.79467 galactic Aql Second-epoch detections are separated by 0.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223059205482633088 | 20:15:41.35 -02:23:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.030 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:41.35 -02:23:51.8: 11.57 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:41.35 -02:23:51.8: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 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 4223059205482633088,2461239.7673,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4223059205482633088 20260718.2673 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.28 20:15:03.28 -02:27:48.4
40.51764 -19.68562 galactic Aql Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.7695-02.4549 | 20:15:03.28 -02:27:48.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.363+/-0.034 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:03.28 -02:27:48.4: 13.15 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:03.28 -02:27:48.4: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 J303.7695-02.4549,2461239.7673,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.7695-02.4549 20260718.2673 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.10 20:15:09.74 -02:23:39.6
40.59585 -19.67691 galactic Aql Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:09.74 -02:23:39.6 (user input) | T | P | (position from user input) J-Ks=0.145+/-0.038 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:09.74 -02:23:39.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:09.74 -02:23:39.6: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.18 20:14:28.84 -02:03:57.9
40.81822 -19.37224 galactic Aql Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4223834906639096064 | 20:14:28.78 -02:03:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.686+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:28.84 -02:03:57.9: 12.15 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:28.84 -02:03:57.9: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 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 4223834906639096064,2461239.7673,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4223834906639096064 20260718.2673 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.98 20:15:23.99 -03:00:21.0
40.05096 -20.01567 galactic Aql Second-epoch detections are separated by 1.1" and 6.6 pix
The object was found in VSX13" ZTF J201524.79-030016.9
Type: EW
# Max. Min./Amp. JD0 Period
16.933 r Y 0.322 r 2458228.95620 0.246920200000
ATTENTION: measured mag 11.98 is 4.6 mag brighter than the VSX record maximum brightness 16.61 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:23.99 -03:00:21.0: 12.90 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:23.99 -03:00:21.0: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ZTF J201524.79-030016.9,2461239.7673,11.98,0.05,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
ZTF J201524.79-030016.9 20260718.2673 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 18.2673 2461239.7673 12.45 20:13:48.46 -03:17:54.0
39.57879 -19.80021 galactic Aql Second-epoch detections are separated by 0.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.992 Swasey 144 111 182 15.0 -0 -0
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:13:48.46 -03:17:54.0: 13.35 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:13:48.46 -03:17:54.0: 13.40 +/- 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
VARIABLE_NAME,2461239.7673,12.45,0.05,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
VARIABLE_NAME 20260718.2673 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 18.2673 2461239.7673 12.44 20:15:18.56 -02:37:14.3
40.40182 -19.81552 galactic Aql Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin -206 -47 211 16.2 -0 -0
ATTENTION: measured mag 12.44 is 3.8 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:18.56 -02:37:14.3: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:18.56 -02:37:14.3: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 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
VARIABLE_NAME,2461239.7673,12.44,0.05,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
VARIABLE_NAME 20260718.2673 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 18.2673 2461239.7673 12.75 20:15:47.35 -02:45:43.9
40.32852 -19.98770 galactic Aql Second-epoch detections are separated by 1.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:47.35 -02:45:43.9 (user input) | T | P | (position from user input) J-Ks=0.711+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:47.35 -02:45:43.9: 14.09 +/- 0.08 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:47.35 -02:45:43.9: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7673,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 11.97 20:16:22.59 -02:35:44.5
40.55822 -20.03920 galactic Aql Second-epoch detections are separated by 0.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:22.59 -02:35:44.5 (user input) | T | P | (position from user input) J-Ks=0.780+/-0.033 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:22.59 -02:35:44.5: 12.90 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:22.59 -02:35:44.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.29 20:15:49.44 -02:25:51.1
40.64409 -19.83997 galactic Aql Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4223058861885207680 | 20:15:49.44 -02:25:51.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.637+/-0.030 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:49.44 -02:25:51.1: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:49.44 -02:25:51.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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
Large-amplitude variable Gaia DR2 4223058861885207680,2461239.7673,12.29,0.05,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
Large-amplitude variable Gaia DR2 4223058861885207680 20260718.2673 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 18.2673 2461239.7673 12.44 20:23:22.12 -04:12:03.1
39.90935 -22.33165 galactic Aql Second-epoch detections are separated by 1.3" and 6.7 pix
The object was found in VSX 1" ASASSN-V J202322.07-041202.2
Type: SR
# Max. Min./Amp. JD0 Period
13.480 V 13.570 V 2456758.00000 319.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:22.12 -04:12:03.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:22.12 -04:12:03.1: 13.41 +/- 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
ASASSN-V J202322.07-041202.2,2461239.7673,12.44,0.05,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 J202322.07-041202.2 20260718.2673 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 18.2673 2461239.7673 10.62 20:15:08.97 -02:37:32.6
40.37717 -19.78264 galactic Aql Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin -349 -65 355 16.2 -0 -0
ATTENTION: measured mag 10.62 is 5.6 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:08.97 -02:37:32.6: 11.41 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:08.97 -02:37:32.6: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 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
VARIABLE_NAME,2461239.7673,10.62,0.05,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
VARIABLE_NAME 20260718.2673 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.40 20:43:37.92 -00:01:47.3
46.55878 -24.75421 galactic Aqr Second-epoch detections are separated by 0.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:37.92 -00:01:47.3 (user input) | T | P | (position from user input) J-Ks=0.619+/-0.034 (K)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:43:37.92 -00:01:47.3: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:43:37.92 -00:01:47.3: 13.38 +/- 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,2461239.7673,12.40,0.05,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 20260718.2673 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.39 20:16:18.20 -02:31:01.4
40.62298 -19.98615 galactic Aql Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.0775-02.5170 | 20:16:18.20 -02:31:01.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.940+/-0.033 (M)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:18.20 -02:31:01.4: 13.32 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:18.20 -02:31:01.4: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 J304.0775-02.5170,2461239.7673,12.39,0.05,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
ATO J304.0775-02.5170 20260718.2673 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 18.2673 2461239.7673 11.86 20:15:33.54 -02:19:06.4
40.71647 -19.72870 galactic Aql Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:33.54 -02:19:06.4 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.030 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:33.54 -02:19:06.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:33.54 -02:19:06.4: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461239.7673,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.2673 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 18.2673 2461239.7673 12.32 20:15:42.22 -02:44:08.0
40.34292 -19.95636 galactic Aql Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin 149 -461 484 16.2 -0 -0
ATTENTION: measured mag 12.32 is 3.9 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:42.22 -02:44:08.0: 13.50 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:42.22 -02:44:08.0: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 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
VARIABLE_NAME,2461239.7673,12.32,0.05,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
VARIABLE_NAME 20260718.2673 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 18.2673 2461239.7673 11.13 20:15:50.06 -02:13:26.2
40.83944 -19.74491 galactic Aql Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9586-02.2239 | 20:15:50.06 -02:13:26.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:50.06 -02:13:26.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:50.06 -02:13:26.2: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 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 J303.9586-02.2239,2461239.7673,11.13,0.05,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
ATO J303.9586-02.2239 20260718.2673 11.13CV 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 18.2673 2461239.7673 12.98 20:38:10.42 +00:12:19.4
46.03405 -23.45499 galactic Aql Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:38:10.42 +00:12:19.4 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.039 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:38:10.42 +00:12:19.4: 14.15 +/- 0.07 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:38:10.42 +00:12:19.4: 14.36 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.7673,12.98,0.05,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 20260718.2673 12.98CV 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 18.2673 2461239.7673 11.93 20:15:39.52 -02:31:07.2
40.54106 -19.84474 galactic Aql Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.5290 Langevin 108 320 338 16.2 -0 -0
ATTENTION: measured mag 11.93 is 4.3 mag brighter than the predicted asteroid brightness 16.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:39.52 -02:31:07.2: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:39.52 -02:31:07.2: 13.12 +/- 0.04 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
VARIABLE_NAME,2461239.7673,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260718.2673 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.2673 2461239.7673 12.17 20:16:31.34 -02:51:47.2
40.32482 -20.19671 galactic Aql Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.1297-02.8659 | 20:16:31.34 -02:51:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.388+/-0.034 (G)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:31.34 -02:51:47.2: 13.12 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:31.34 -02:51:47.2: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 J304.1297-02.8659,2461239.7673,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.1297-02.8659 20260718.2673 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461212.86349038 21.06.2026 08:43:15.569 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
First image: 2461212.86349038 21.06.2026 08:43:15.569 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Last image: 2461239.76760079 18.07.2026 06:25:10.708 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11398
Objects passed selection criteria: 11325
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 6580.25
Average stars matched: 6332.25 (96.2311 %)
Memory usage VmPeak: 121052 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 06:58:31 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: 2461212.86349038 21.06.2026 08:43:15.569 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
First image: 2461212.86349038 21.06.2026 08:43:15.569 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Last image: 2461239.76760079 18.07.2026 06:25:10.708 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 112
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 88133
Objects passed selection criteria: 87847
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: 55554
Average stars matched: 52826.2 (95.0899 %)
Memory usage VmPeak: 1865548 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 07:03:13 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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
SExtractor catalog cache: saved Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.cat to cache
SExtractor catalog cache: saved Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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: 2461239.76693241
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits exists and is non-empty
Saving wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits to local_wcs_cache/
'wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits' -> 'local_wcs_cache/wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits'
wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits exists and is non-empty
Saving wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits to local_wcs_cache/
'wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits' -> 'local_wcs_cache/wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits'
wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits'
wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits exists and is non-empty
Saving wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits to local_wcs_cache/
'wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits (1st reference image)
verification OK: wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Image size: 937.0'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: 20:34:16.807 -01:59:52.55 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-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits (1st new image)
verification OK: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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: 20:34:16.932 -02:00:45.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:16.807 -01:59:52.55
Second-epoch image center 20:34:16.932 -02:00:45.62
Angular distance between the image centers 0.0148 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits (2nd new image)
verification OK: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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: 20:34:19.079 -02:01:08.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:16.807 -01:59:52.55
Second-epoch image center 20:34:19.079 -02:01:08.09
Angular distance between the image centers 0.0230 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 20:34:16.932 -02:00:45.62
Second-epoch second image center 20:34:19.079 -02:01:08.09
Angular distance between the image centers 0.01090 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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits &> /tmp/tmp.8prPsiRQJJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits &> /tmp/tmp.vDDLcY40fD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits &> /tmp/tmp.LTrJtyieJ6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits &> /tmp/tmp.C4847HsZvT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits and wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits and wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat
Found non-empty wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits and wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat
The reference image (wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits) and catalog (wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat) found
'wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat' -> 'wcsmag.cat'
Read 15228 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.7161 to 316.4569 deg, Dec -7.2646 to +3.2719 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 300.7161 to 316.4569 deg, Dec -7.2646 to 3.2719 deg
Loaded 10829 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): 8829 out of 9264 total matches.
Matched with Tycho-2 9264 out of 15228 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.702500
a=0.000000 b=1.000000 c=22.702500
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 15228 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.7161 to 316.4569 deg, Dec -7.2646 to +3.2719 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 300.7161 to 316.4569 deg, Dec -7.2646 to 3.2719 deg
Loaded 10829 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): 8829 out of 9264 total matches.
Matched with Tycho-2 9264 out of 15228 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits:
Forced-photometry filter: calibrated wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits -> calib.txt_param_ref_wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits (aperture=6.1)
Read 15674 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.7162 to 316.4583 deg, Dec -7.2811 to +3.2571 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 300.7162 to 316.4583 deg, Dec -7.2811 to 3.2571 deg
Loaded 10825 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): 8861 out of 9345 total matches.
Matched with Tycho-2 9345 out of 15674 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits:
Forced-photometry filter: calibrated wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits -> calib.txt_param_ref_wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
2.3 pix Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
2.3 pix fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
2.2 pix fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
2.3 pix wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
2.3 pix wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Limiting magnitude estimates:
15.0 mag. Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
15.0 mag. Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
12.1 mag. fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
12.8 mag. fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
All-image limiting magnitude estimate: 12.1 (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.8prPsiRQJJ (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits' -> 'wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
WCS-calibrated image found: wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Checking if the catalog wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
WCS catalog name: wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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=1000, bad_region=3112, passed=15228
Got 15228 stars (including 11294 good ones) from the SExtractor catalog wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 15228 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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12468 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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits N_match=959 sigma_overall_arcsec=0.505 sigma_q1_arcsec=0.438 sigma_q2_arcsec=0.610 sigma_q3_arcsec=0.502 sigma_q4_arcsec=0.533 n_q1=295 n_q2=184 n_q3=298 n_q4=182 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits -region wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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.vDDLcY40fD (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits' -> 'wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
WCS_IMAGE_NAME=wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
WCS-calibrated image found: wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Checking if the catalog wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits alredy exist and is non-empty...
Catalog wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
WCS catalog name: wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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=1089, bad_region=3208, passed=15674
Got 15674 stars (including 11577 good ones) from the SExtractor catalog wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat
util/solve_plate_with_UCAC5 got 15674 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 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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=Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits N_match=960 sigma_overall_arcsec=0.439 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.486 sigma_q3_arcsec=0.481 sigma_q4_arcsec=0.472 n_q1=293 n_q2=178 n_q3=311 n_q4=178 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits -region wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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.LTrJtyieJ6 (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
Checking if the catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
WCS catalog name: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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=48, bad_region=217, passed=1045
Got 1045 stars (including 788 good ones) from the SExtractor catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat
util/solve_plate_with_UCAC5 got 1045 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 739 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 734 matched stars entering correct_measured_positions(), 694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 734 matched stars entering correct_measured_positions(), 798 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 739 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 734 matched stars entering correct_measured_positions(), 798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 734 matched stars entering correct_measured_positions(), 798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 734 stars left (next iteration limit 807)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits N_match=734 sigma_overall_arcsec=0.588 sigma_q1_arcsec=0.536 sigma_q2_arcsec=0.609 sigma_q3_arcsec=0.617 sigma_q4_arcsec=0.513 n_q1=232 n_q2=180 n_q3=173 n_q4=149 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits -region wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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.C4847HsZvT (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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=73, bad_region=296, passed=1373
Got 1373 stars (including 1020 good ones) from the SExtractor catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat
util/solve_plate_with_UCAC5 got 1373 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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1054 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 3.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 1052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 1052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 948 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits N_match=948 sigma_overall_arcsec=0.523 sigma_q1_arcsec=0.463 sigma_q2_arcsec=0.567 sigma_q3_arcsec=0.518 sigma_q4_arcsec=0.562 n_q1=293 n_q2=241 n_q3=254 n_q4=160 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits -region wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits sigma_overall=0.505 worst_q_ratio=1.206
ref2=Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits sigma_overall=0.439 worst_q_ratio=1.108
new1=fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits sigma_overall=0.588 worst_q_ratio=1.049
new2=fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits sigma_overall=0.523 worst_q_ratio=1.083
reference average sigma_overall=0.472 worst_q_ratio=1.157
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366_astrometric_residuals.png (959 matched stars from wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370_astrometric_residuals.png (960 matched stars from wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228_astrometric_residuals.png (734 matched stars from wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229_astrometric_residuals.png (948 matched stars from wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits'
Preparing the HTML report for the field Aql-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aql-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
SExtractor catalog cache: saved Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.cat to cache
SExtractor catalog cache: saved Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Creating symlink local_wcs_cache/wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits exists and is non-empty
wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits exists and is non-empty
wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits (1st reference image)
verification OK: wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Image size: 937.0'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: 20:34:16.807 -01:59:52.55 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-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits (1st new image)
verification OK: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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: 20:34:16.932 -02:00:45.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:16.807 -01:59:52.55
Second-epoch image center 20:34:16.932 -02:00:45.62
Angular distance between the image centers 0.0148 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits (2nd new image)
verification OK: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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: 20:34:19.079 -02:01:08.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:16.807 -01:59:52.55
Second-epoch image center 20:34:19.079 -02:01:08.09
Angular distance between the image centers 0.0230 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 20:34:16.932 -02:00:45.62
Second-epoch second image center 20:34:19.079 -02:01:08.09
Angular distance between the image centers 0.01090 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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits &> /tmp/tmp.AclqyHzHmz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits &> /tmp/tmp.Gzz9ikP6cD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits &> /tmp/tmp.lt6QXVxBdZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits &> /tmp/tmp.YZHx5GUgU0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits and wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits and wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat
Found non-empty wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits and wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat
The reference image (wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits) and catalog (wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat) found
'wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat' -> 'wcsmag.cat'
Read 111374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.7123 to 316.4570 deg, Dec -7.2649 to +3.2733 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 300.7123 to 316.4570 deg, Dec -7.2649 to 3.2733 deg
Loaded 10831 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): 8130 out of 9765 total matches.
Matched with Tycho-2 9765 out of 111374 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.546700
a=0.000000 b=1.000000 c=22.546700
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 111374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.7123 to 316.4570 deg, Dec -7.2649 to +3.2733 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 300.7123 to 316.4570 deg, Dec -7.2649 to 3.2733 deg
Loaded 10831 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): 8130 out of 9765 total matches.
Matched with Tycho-2 9765 out of 111374 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits:
Forced-photometry filter: calibrated wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits -> calib.txt_param_ref_wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits (aperture=4.6)
Read 116458 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.7116 to 316.4605 deg, Dec -7.2812 to +3.2590 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 300.7116 to 316.4605 deg, Dec -7.2812 to 3.2590 deg
Loaded 10829 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): 7940 out of 9760 total matches.
Matched with Tycho-2 9760 out of 116458 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits:
Forced-photometry filter: calibrated wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits -> calib.txt_param_ref_wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 98 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
2.1 pix Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
2.1 pix fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
2.0 pix fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
2.1 pix wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
2.1 pix wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Limiting magnitude estimates:
15.2 mag. Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
15.2 mag. Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
12.9 mag. fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
13.4 mag. fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.6 (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.AclqyHzHmz (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits' -> 'wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
WCS-calibrated image found: wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
Checking if the catalog wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits
WCS catalog name: wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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=19, blended=9199, bad_region=14235, passed=111355
Got 111355 stars (including 89111 good ones) from the SExtractor catalog wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 111355 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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 98706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 98706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 98704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits N_match=954 sigma_overall_arcsec=0.461 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.521 sigma_q3_arcsec=0.484 sigma_q4_arcsec=0.515 n_q1=295 n_q2=175 n_q3=293 n_q4=191 worst_quadrant_to_overall_ratio=1.131
The image catalog is written to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits -region wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.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.Gzz9ikP6cD (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits' -> 'wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
WCS_IMAGE_NAME=wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
WCS-calibrated image found: wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
Checking if the catalog wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits alredy exist and is non-empty...
Catalog wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat corresponding to the image wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits
WCS catalog name: wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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=27, blended=9969, bad_region=16899, passed=116431
Got 116431 stars (including 90648 good ones) from the SExtractor catalog wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat
util/solve_plate_with_UCAC5 got 116431 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 3.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 101221 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 101221 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 101220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits N_match=956 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.477 sigma_q4_arcsec=0.465 n_q1=291 n_q2=187 n_q3=290 n_q4=188 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits -region wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.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.lt6QXVxBdZ (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
Checking if the catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
WCS catalog name: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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=2, blended=340, bad_region=1526, passed=13186
Got 13186 stars (including 11362 good ones) from the SExtractor catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat
util/solve_plate_with_UCAC5 got 13186 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 3.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 11328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 11328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 11321 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 930 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits N_match=930 sigma_overall_arcsec=0.514 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.545 sigma_q3_arcsec=0.548 sigma_q4_arcsec=0.496 n_q1=310 n_q2=193 n_q3=217 n_q4=210 worst_quadrant_to_overall_ratio=1.068
The image catalog is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits -region wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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.YZHx5GUgU0 (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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
Checking if the catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat corresponding to the image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
WCS catalog name: wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=635, bad_region=2284, passed=17716
Got 17716 stars (including 14950 good ones) from the SExtractor catalog wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat
util/solve_plate_with_UCAC5 got 17716 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 3.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 14906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 14904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 14904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits N_match=949 sigma_overall_arcsec=0.497 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.563 sigma_q3_arcsec=0.529 sigma_q4_arcsec=0.502 n_q1=301 n_q2=221 n_q3=253 n_q4=174 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Aql-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits -region wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-24-12_20.00sec_5.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.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-05-Q2b1x1_021256_TTUQ2b1x1_3671488_nySSbOzB/wcs_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229.fits
Preparing the HTML report for the field Aql-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:47:39.34 -04:59:23.4: 12.00 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:46.13 -04:11:11.4: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:43:36.06 -00:01:45.2: 13.52 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:36:36.83 +00:16:14.5: 13.32 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:38.50 +00:00:54.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:20.76 -02:29:11.0: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:31.57 -02:48:05.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:06.46 -02:56:32.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:36:48.45 +00:16:39.5: 13.67 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:47:39.34 -04:59:23.4: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter REJECTED candidate at 20:47:39.34 -04:59:23.4: ref_mag=11.91 +/- 0.01 new_mean_mag=11.7892 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:39:57.41 +00:21:22.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:46.13 -04:11:11.4: 13.50 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:43:36.06 -00:01:45.2: 13.44 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:36:36.83 +00:16:14.5: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 20:23:46.13 -04:11:11.4: ref_mag=13.42 +/- 0.03 new_mean_mag=12.3361 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter KEPT candidate at 20:43:36.06 -00:01:45.2: ref_mag=13.48 +/- 0.03 new_mean_mag=12.4533 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 20:36:36.83 +00:16:14.5: ref_mag=13.31 +/- 0.03 new_mean_mag=12.3169 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:31.57 -02:48:05.6: 13.10 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:20.76 -02:29:11.0: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 20:16:31.57 -02:48:05.6: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1121 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:38.50 +00:00:54.3: 13.16 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:36:48.45 +00:16:39.5: 13.70 +/- 0.05 detection
Forced photometry filter KEPT candidate at 20:16:20.76 -02:29:11.0: ref_mag=13.41 +/- 0.03 new_mean_mag=12.2944 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:06.46 -02:56:32.1: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 20:36:48.45 +00:16:39.5: ref_mag=13.68 +/- 0.04 new_mean_mag=12.6234 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 20:37:38.50 +00:00:54.3: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1567 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:06.46 -02:56:32.1: ref_mag=13.42 +/- 0.03 new_mean_mag=12.3878 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:39:57.41 +00:21:22.6: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 20:39:57.41 +00:21:22.6: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7483 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:19.38 +00:10:11.5: 12.19 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:19.38 +00:10:11.5: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 20:37:19.38 +00:10:11.5: ref_mag=12.20 +/- 0.01 new_mean_mag=11.2175 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:52.15 -02:15:14.8: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:29.40 -03:06:16.4: 12.20 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:52.15 -02:15:14.8: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:52.15 -02:15:14.8: ref_mag=13.18 +/- 0.03 new_mean_mag=12.0340 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:29.40 -03:06:16.4: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:29.40 -03:06:16.4: ref_mag=12.25 +/- 0.01 new_mean_mag=11.2898 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:24:11.19 -04:12:05.7: 11.70 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:24:11.19 -04:12:05.7: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Forced photometry filter KEPT candidate at 20:24:11.19 -04:12:05.7: ref_mag=11.69 +/- 0.01 new_mean_mag=10.7860 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:54.83 -02:17:07.2: 11.76 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:01.73 -03:07:21.6: 13.21 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:54.83 -02:17:07.2: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:54.83 -02:17:07.2: ref_mag=11.78 +/- 0.01 new_mean_mag=10.8132 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:01.73 -03:07:21.6: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:01.73 -03:07:21.6: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2115 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:56.65 -04:09:32.4: 13.23 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:33.59 -02:06:17.0: 13.43 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:46.96 -02:21:54.7: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:56.65 -04:09:32.4: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 20:23:56.65 -04:09:32.4: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1705 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:33.59 -02:06:17.0: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:33.59 -02:06:17.0: ref_mag=13.44 +/- 0.03 new_mean_mag=12.4037 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:42.25 -02:50:35.1: 13.78 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:46.96 -02:21:54.7: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:46.96 -02:21:54.7: ref_mag=13.07 +/- 0.02 new_mean_mag=11.9148 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:37.61 +00:00:28.4: 13.26 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:42.25 -02:50:35.1: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter KEPT candidate at 20:15:42.25 -02:50:35.1: ref_mag=13.76 +/- 0.04 new_mean_mag=12.5100 delta=1.25 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:37.61 +00:00:28.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 20:37:37.61 +00:00:28.4: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2687 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:11.07 -02:44:06.9: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:11.07 -02:44:06.9: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:11.07 -02:44:06.9: ref_mag=13.27 +/- 0.03 new_mean_mag=12.1947 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:57.81 -02:22:40.1: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:57.81 -02:22:40.1: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:57.81 -02:22:40.1: ref_mag=13.29 +/- 0.03 new_mean_mag=12.0210 delta=1.27 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:35.57 -00:01:18.0: 13.80 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:38:07.64 +00:19:55.7: 13.76 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:35.57 -00:01:18.0: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter KEPT candidate at 20:37:35.57 -00:01:18.0: ref_mag=13.79 +/- 0.04 new_mean_mag=12.7690 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:38:07.64 +00:19:55.7: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry filter KEPT candidate at 20:38:07.64 +00:19:55.7: ref_mag=13.80 +/- 0.04 new_mean_mag=12.7699 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:30.57 -04:14:23.9: 12.81 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:30.57 -04:14:23.9: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter KEPT candidate at 20:23:30.57 -04:14:23.9: ref_mag=12.81 +/- 0.02 new_mean_mag=11.8806 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:38:48.40 +00:18:30.8: 13.79 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:38:48.40 +00:18:30.8: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 20:38:48.40 +00:18:30.8: ref_mag=13.78 +/- 0.04 new_mean_mag=12.7133 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:31.14 -02:21:26.8: 13.65 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:31.14 -02:21:26.8: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 20:15:31.14 -02:21:26.8: ref_mag=13.65 +/- 0.04 new_mean_mag=12.5247 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:06.12 -02:36:09.6: 13.27 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:36.95 -02:13:04.3: 13.25 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:06.12 -02:36:09.6: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:06.12 -02:36:09.6: ref_mag=13.27 +/- 0.03 new_mean_mag=12.1871 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:36.95 -02:13:04.3: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:36.95 -02:13:04.3: ref_mag=13.25 +/- 0.02 new_mean_mag=12.1848 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:13:58.83 -03:12:40.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:13:58.83 -03:12:40.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 20:13:58.83 -03:12:40.4: ref_mag=13.45 +/- 0.03 new_mean_mag=12.2633 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:19.37 +00:00:11.1: 14.15 +/- 0.07 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:19.37 +00:00:11.1: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Forced photometry filter KEPT candidate at 20:37:19.37 +00:00:11.1: ref_mag=14.05 +/- 0.05 new_mean_mag=12.9320 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:03.62 -02:36:58.2: 12.80 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:03.62 -02:36:58.2: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 20:16:03.62 -02:36:58.2: ref_mag=12.87 +/- 0.02 new_mean_mag=11.8678 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:05.66 -02:28:02.1: 13.43 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:05.66 -02:28:02.1: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:05.66 -02:28:02.1: ref_mag=13.38 +/- 0.03 new_mean_mag=12.2652 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:05.93 -02:56:55.1: 13.06 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:05.93 -02:56:55.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 20:16:05.93 -02:56:55.1: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1228 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:43.14 -02:36:01.6: 13.07 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:43.14 -02:36:01.6: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 20:14:43.14 -02:36:01.6: ref_mag=13.05 +/- 0.02 new_mean_mag=11.9845 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:21.22 -01:57:46.7: 12.41 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:48.53 -04:14:03.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:21.22 -01:57:46.7: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter KEPT candidate at 20:14:21.22 -01:57:46.7: ref_mag=12.46 +/- 0.01 new_mean_mag=11.5042 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:48.53 -04:14:03.1: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 20:23:48.53 -04:14:03.1: ref_mag=13.06 +/- 0.02 new_mean_mag=11.9126 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:39.55 -04:14:24.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:39.55 -04:14:24.3: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 20:23:39.55 -04:14:24.3: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0226 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:20.88 -02:48:06.9: 13.25 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:44.99 -02:44:46.7: 13.23 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:20.88 -02:48:06.9: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:20.88 -02:48:06.9: ref_mag=13.27 +/- 0.03 new_mean_mag=12.1616 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:44.99 -02:44:46.7: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:44.99 -02:44:46.7: ref_mag=13.24 +/- 0.03 new_mean_mag=12.1871 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:32.14 -02:58:22.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:32.14 -02:58:22.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:32.14 -02:58:22.3: ref_mag=13.05 +/- 0.02 new_mean_mag=11.8422 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:54.39 -02:22:34.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:54.39 -02:22:34.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:54.39 -02:22:34.8: ref_mag=12.78 +/- 0.02 new_mean_mag=11.5870 delta=1.20 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:22.65 -02:26:19.2: 13.42 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:54.16 -02:12:26.6: 13.41 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:22.65 -02:26:19.2: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:22.65 -02:26:19.2: ref_mag=13.50 +/- 0.03 new_mean_mag=12.3167 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:54.16 -02:12:26.6: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:54.16 -02:12:26.6: ref_mag=13.42 +/- 0.03 new_mean_mag=12.3355 delta=1.09 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:28.95 -02:25:48.0: 12.74 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:03.80 -02:20:06.7: 13.38 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:28.95 -02:25:48.0: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:28.95 -02:25:48.0: ref_mag=12.80 +/- 0.02 new_mean_mag=11.7219 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:03.80 -02:20:06.7: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:03.80 -02:20:06.7: ref_mag=13.41 +/- 0.03 new_mean_mag=12.2126 delta=1.20 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:32.62 -02:56:38.8: 13.23 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:32.62 -02:56:38.8: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:32.62 -02:56:38.8: ref_mag=13.23 +/- 0.03 new_mean_mag=12.0961 delta=1.14 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:24.24 -02:21:57.1: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:24.24 -02:21:57.1: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:24.24 -02:21:57.1: ref_mag=13.03 +/- 0.02 new_mean_mag=11.9796 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:21.09 -02:54:29.5: 13.24 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:21.09 -02:54:29.5: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:21.09 -02:54:29.5: ref_mag=13.27 +/- 0.03 new_mean_mag=12.2639 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:51.41 -02:27:26.6: 12.70 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:51.41 -02:27:26.6: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:51.41 -02:27:26.6: ref_mag=12.73 +/- 0.02 new_mean_mag=11.7079 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:24.74 -02:50:50.2: 13.20 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:24.74 -02:50:50.2: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:24.74 -02:50:50.2: ref_mag=13.18 +/- 0.03 new_mean_mag=12.0450 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:16.12 -03:11:57.0: 12.32 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:37:26.59 +00:07:23.6: 13.73 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:16.12 -03:11:57.0: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 20:14:16.12 -03:11:57.0: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3878 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:37:26.59 +00:07:23.6: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter KEPT candidate at 20:37:26.59 +00:07:23.6: ref_mag=13.68 +/- 0.04 new_mean_mag=12.5859 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:28.25 -02:21:20.0: 13.73 +/- 0.06 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:28.25 -02:21:20.0: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 20:15:28.25 -02:21:20.0: ref_mag=13.72 +/- 0.04 new_mean_mag=12.4982 delta=1.22 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:52.21 -03:10:30.0: 12.94 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:52.21 -03:10:30.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 20:14:52.21 -03:10:30.0: ref_mag=12.98 +/- 0.02 new_mean_mag=12.0447 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:04.32 -02:26:07.7: 12.30 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:04.32 -02:26:07.7: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:04.32 -02:26:07.7: ref_mag=12.32 +/- 0.01 new_mean_mag=11.3528 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:56.24 -04:17:37.3: 12.29 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:56.24 -04:17:37.3: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 20:23:56.24 -04:17:37.3: ref_mag=12.30 +/- 0.01 new_mean_mag=11.3599 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:34.94 -03:07:41.5: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:34.94 -03:07:41.5: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 20:14:34.94 -03:07:41.5: ref_mag=12.30 +/- 0.01 new_mean_mag=11.3783 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:59.41 -02:20:20.6: 11.75 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:59.41 -02:20:20.6: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:59.41 -02:20:20.6: ref_mag=11.77 +/- 0.01 new_mean_mag=10.7460 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:48.69 -02:12:45.0: 12.28 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:48.69 -02:12:45.0: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:48.69 -02:12:45.0: ref_mag=12.33 +/- 0.01 new_mean_mag=11.3102 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:08.67 -02:05:03.4: 12.67 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:08.67 -02:05:03.4: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:08.67 -02:05:03.4: ref_mag=12.73 +/- 0.02 new_mean_mag=11.7925 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:17.31 -03:10:38.9: 12.25 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:17.31 -03:10:38.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 20:14:17.31 -03:10:38.9: ref_mag=12.28 +/- 0.01 new_mean_mag=11.3421 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:11.65 -02:14:55.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:11.65 -02:14:55.3: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:11.65 -02:14:55.3: ref_mag=13.21 +/- 0.02 new_mean_mag=12.1352 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:30.95 -02:42:46.9: 13.18 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:59.73 -03:05:25.5: 12.93 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:30.95 -02:42:46.9: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:30.95 -02:42:46.9: ref_mag=13.23 +/- 0.03 new_mean_mag=12.1263 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:59.73 -03:05:25.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 20:14:59.73 -03:05:25.5: ref_mag=12.90 +/- 0.02 new_mean_mag=11.8643 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:23.51 -02:25:46.8: 12.94 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:23.51 -02:25:46.8: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:23.51 -02:25:46.8: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9198 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:07.67 -02:50:01.0: 13.70 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:40.01 -02:56:51.0: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:07.67 -02:50:01.0: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 20:16:07.67 -02:50:01.0: ref_mag=13.69 +/- 0.04 new_mean_mag=12.6328 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:40.01 -02:56:51.0: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:40.01 -02:56:51.0: ref_mag=13.17 +/- 0.03 new_mean_mag=12.0529 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:29.25 -03:03:15.6: 13.18 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:29.25 -03:03:15.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:29.25 -03:03:15.6: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1951 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:43:43.71 +00:01:32.6: 13.50 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:43:43.71 +00:01:32.6: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter REJECTED candidate at 20:43:43.71 +00:01:32.6: ref_mag=13.48 +/- 0.03 new_mean_mag=12.5976 delta=0.88 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:43.53 -02:27:24.4: 11.60 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:43.53 -02:27:24.4: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:43.53 -02:27:24.4: ref_mag=11.62 +/- 0.01 new_mean_mag=10.6891 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:13:59.50 -01:57:29.9: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:13:59.50 -01:57:29.9: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 20:13:59.50 -01:57:29.9: ref_mag=12.66 +/- 0.02 new_mean_mag=11.6889 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:13.24 -01:54:59.0: 12.19 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:13.24 -01:54:59.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 20:14:13.24 -01:54:59.0: ref_mag=12.23 +/- 0.01 new_mean_mag=11.3030 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:02.84 -02:33:54.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:09.85 -02:42:23.3: 12.63 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:02.84 -02:33:54.1: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:02.84 -02:33:54.1: ref_mag=12.23 +/- 0.01 new_mean_mag=11.2757 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:09.85 -02:42:23.3: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:09.85 -02:42:23.3: ref_mag=12.61 +/- 0.02 new_mean_mag=11.6161 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:41.35 -02:23:51.8: 11.57 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:41.35 -02:23:51.8: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:41.35 -02:23:51.8: ref_mag=11.59 +/- 0.01 new_mean_mag=10.6803 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:03.28 -02:27:48.4: 13.15 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:09.74 -02:23:39.6: 13.15 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:03.28 -02:27:48.4: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:03.28 -02:27:48.4: ref_mag=13.22 +/- 0.03 new_mean_mag=12.2077 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:09.74 -02:23:39.6: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:09.74 -02:23:39.6: ref_mag=13.16 +/- 0.02 new_mean_mag=12.0615 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:28.84 -02:03:57.9: 12.15 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:28.84 -02:03:57.9: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter KEPT candidate at 20:14:28.84 -02:03:57.9: ref_mag=12.19 +/- 0.01 new_mean_mag=11.1904 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:23.99 -03:00:21.0: 12.90 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:13:48.46 -03:17:54.0: 13.35 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:23.99 -03:00:21.0: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:23.99 -03:00:21.0: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9180 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:13:48.46 -03:17:54.0: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 20:13:48.46 -03:17:54.0: ref_mag=13.38 +/- 0.03 new_mean_mag=12.4498 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:18.56 -02:37:14.3: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:18.56 -02:37:14.3: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry filter KEPT candidate at 20:15:18.56 -02:37:14.3: ref_mag=13.55 +/- 0.04 new_mean_mag=12.4732 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:47.35 -02:45:43.9: 14.09 +/- 0.08 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:47.35 -02:45:43.9: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.06
Forced photometry filter KEPT candidate at 20:15:47.35 -02:45:43.9: ref_mag=14.09 +/- 0.06 new_mean_mag=12.7534 delta=1.34 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:49.44 -02:25:51.1: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:22.59 -02:35:44.5: 12.90 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:23:22.12 -04:12:03.1: 13.35 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:49.44 -02:25:51.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:49.44 -02:25:51.1: ref_mag=13.37 +/- 0.03 new_mean_mag=12.2921 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:23:22.12 -04:12:03.1: 13.41 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:22.59 -02:35:44.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 20:23:22.12 -04:12:03.1: ref_mag=13.38 +/- 0.03 new_mean_mag=12.4351 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 20:16:22.59 -02:35:44.5: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9980 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:08.97 -02:37:32.6: 11.41 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:08.97 -02:37:32.6: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Forced photometry filter KEPT candidate at 20:15:08.97 -02:37:32.6: ref_mag=11.43 +/- 0.00 new_mean_mag=10.4870 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:43:37.92 -00:01:47.3: 13.34 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:43:37.92 -00:01:47.3: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 20:43:37.92 -00:01:47.3: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4232 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:18.20 -02:31:01.4: 13.32 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:18.20 -02:31:01.4: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:18.20 -02:31:01.4: ref_mag=13.39 +/- 0.03 new_mean_mag=12.4081 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:33.54 -02:19:06.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:33.54 -02:19:06.4: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:33.54 -02:19:06.4: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8910 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:42.22 -02:44:08.0: 13.50 +/- 0.05 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:42.22 -02:44:08.0: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 20:15:42.22 -02:44:08.0: ref_mag=13.49 +/- 0.03 new_mean_mag=12.3762 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:50.06 -02:13:26.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:50.06 -02:13:26.2: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter KEPT candidate at 20:15:50.06 -02:13:26.2: ref_mag=12.09 +/- 0.01 new_mean_mag=11.1431 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:38:10.42 +00:12:19.4: 14.15 +/- 0.07 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:38:10.42 +00:12:19.4: 14.36 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Forced photometry filter KEPT candidate at 20:38:10.42 +00:12:19.4: ref_mag=14.24 +/- 0.06 new_mean_mag=12.9950 delta=1.24 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:15:39.52 -02:31:07.2: 13.09 +/- 0.03 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:15:39.52 -02:31:07.2: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 20:15:39.52 -02:31:07.2: ref_mag=13.11 +/- 0.02 new_mean_mag=11.9489 delta=1.16 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:16:31.34 -02:51:47.2: 13.12 +/- 0.04 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:16:31.34 -02:51:47.2: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:31.34 -02:51:47.2: ref_mag=13.19 +/- 0.03 new_mean_mag=12.1797 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-21_03-43-15_20.00sec_4.90C_LIGHT_0366.fits at 20:14:14.05 -01:54:36.6: 12.78 +/- 0.02 detection
Forced photometry on wcs_Aql-05-Q2b1x1_2026-06-22_03-34-34_20.00sec_4.90C_LIGHT_0370.fits at 20:14:14.05 -01:54:36.6: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter REJECTED candidate at 20:14:14.05 -01:54:36.6: ref_mag=12.80 +/- 0.02 new_mean_mag=11.9077 delta=0.89 (need > 0.90)
Adding exclusion_list_local.txt__out104376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80951.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 126s
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: 63s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132193_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
The candidate 132193_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
**** FOUND 20:38:53.07 -03:51:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132205_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
The candidate 132205_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104965_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 104965_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39250_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 39250_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44178_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44178_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40740_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 40740_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105064_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 105064_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26576_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26576_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80855_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80855_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80951_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80951_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79961_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 79961_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80465_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80465_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46802_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 46802_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37429_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 37429_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26320_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26320_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46286_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 46286_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37234_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 37234_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26829_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26829_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48458_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48458_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45530_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45530_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40375_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 40375_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80857_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80857_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41519_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 41519_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45425_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45425_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80936_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80936_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104376_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 104376_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26096_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26096_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104645_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 104645_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45631_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45631_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42982_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 42982_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47267_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47267_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36387_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 36387_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107081_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 107081_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42738_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 42738_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44438_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44438_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39129_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 39129_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43016_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 43016_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49877_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 49877_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26107_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26107_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26095_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26095_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40780_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 40780_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41416_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 41416_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38852_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 38852_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45377_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45377_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47345_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47345_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44739_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44739_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44840_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44840_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45894_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45894_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39241_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 39241_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45531_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45531_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39615_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 39615_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44494_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44494_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40276_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 40276_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36388_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 36388_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106162_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 106162_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45651_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45651_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36677_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 36677_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44721_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44721_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25470_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 25470_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37151_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 37151_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45759_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45759_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47219_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47219_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48638_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48638_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36599_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 36599_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46877_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 46877_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41740_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 41740_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37572_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 37572_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44833_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44833_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40438_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 40438_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39130_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 39130_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38008_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 38008_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80850_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
The candidate 80850_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44409_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44409_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50046_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 50046_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50494_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 50494_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43276_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 43276_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41770_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 41770_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45003_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45003_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44486_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44486_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45211_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 45211_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48797_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 48797_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38460_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 38460_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35446_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 35446_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42768_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 42768_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41273_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 41273_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43038_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 43038_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44818_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 44818_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26447_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 26447_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42639_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 42639_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80948_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80948_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43878_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 43878_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46023_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 46023_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41545_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 41545_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47065_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 47065_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80336_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 80336_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43898_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 43898_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40031_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
Preparing report for the candidate 40031_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50602_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229
The candidate 50602_fd_Aql-05-Q2b1x1_2026-07-18_01-25-10_20.00sec_5.00C_LIGHT_0229 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 196s
Prepared the HTML report for the field Aql-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:38:07.64 +00:19:55.7
20:38:48.40 +00:18:30.8
20:36:36.83 +00:16:14.5
20:36:48.45 +00:16:39.5
20:37:26.59 +00:07:23.6
20:37:19.37 +00:00:11.1
20:23:56.24 -04:17:37.3
20:23:39.55 -04:14:24.3
20:23:30.57 -04:14:23.9
20:23:48.53 -04:14:03.1
20:24:11.19 -04:12:05.7
20:23:22.12 -04:12:03.1
20:23:46.13 -04:11:11.4
20:23:56.65 -04:09:32.4
20:13:48.46 -03:17:54.0
20:13:58.83 -03:12:40.4
20:14:16.12 -03:11:57.0
20:14:17.31 -03:10:38.9
20:14:52.21 -03:10:30.0
20:14:34.94 -03:07:41.5
20:15:01.73 -03:07:21.6
20:15:29.40 -03:06:16.4
20:14:59.73 -03:05:25.5
20:15:29.25 -03:03:15.6
20:15:23.99 -03:00:21.0
20:15:32.14 -02:58:22.3
20:16:05.93 -02:56:55.1
20:15:40.01 -02:56:51.0
20:15:32.62 -02:56:38.8
20:16:06.46 -02:56:32.1
20:16:21.09 -02:54:29.5
20:16:31.34 -02:51:47.2
20:15:24.74 -02:50:50.2
20:15:42.25 -02:50:35.1
20:16:07.67 -02:50:01.0
20:16:31.57 -02:48:05.6
20:15:20.88 -02:48:06.9
20:15:47.35 -02:45:43.9
20:15:44.99 -02:44:46.7
20:16:11.07 -02:44:06.9
20:15:42.22 -02:44:08.0
20:15:30.95 -02:42:46.9
20:15:09.85 -02:42:23.3
20:15:08.97 -02:37:32.6
20:16:03.62 -02:36:58.2
20:15:18.56 -02:37:14.3
20:15:06.12 -02:36:09.6
20:14:43.14 -02:36:01.6
20:16:22.59 -02:35:44.5
20:15:02.84 -02:33:54.1
20:16:18.20 -02:31:01.4
20:15:39.52 -02:31:07.2
20:16:20.76 -02:29:11.0
20:15:43.53 -02:27:24.4
20:16:05.66 -02:28:02.1
20:15:03.28 -02:27:48.4
20:15:51.41 -02:27:26.6
20:15:04.32 -02:26:07.7
20:15:22.65 -02:26:19.2
20:15:49.44 -02:25:51.1
20:15:23.51 -02:25:46.8
20:15:28.95 -02:25:48.0
20:15:41.35 -02:23:51.8
20:15:09.74 -02:23:39.6
20:15:54.39 -02:22:34.8
20:15:57.81 -02:22:40.1
20:15:46.96 -02:21:54.7
20:15:24.24 -02:21:57.1
20:15:31.14 -02:21:26.8
20:15:28.25 -02:21:20.0
20:15:59.41 -02:20:20.6
20:16:03.80 -02:20:06.7
20:15:33.54 -02:19:06.4
20:15:54.83 -02:17:07.2
20:15:52.15 -02:15:14.8
20:15:11.65 -02:14:55.3
20:15:50.06 -02:13:26.2
20:15:48.69 -02:12:45.0
20:15:36.95 -02:13:04.3
20:15:54.16 -02:12:26.6
20:15:33.59 -02:06:17.0
20:15:08.67 -02:05:03.4
20:14:28.84 -02:03:57.9
20:14:21.22 -01:57:46.7
20:13:59.50 -01:57:29.9
20:14:13.24 -01:54:59.0
20:39:57.41 +00:21:22.6
20:38:10.42 +00:12:19.4
20:37:19.38 +00:10:11.5
20:37:38.50 +00:00:54.3
20:37:37.61 +00:00:28.4
20:37:35.57 -00:01:18.0
20:43:37.92 -00:01:47.3
20:43:36.06 -00:01:45.2
########### Completed Aql-05-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 ####
20:36:36.83 +00:16:14.5
20:16:06.46 -02:56:32.1
20:16:20.76 -02:29:11.0
20:16:31.57 -02:48:05.6
20:36:48.45 +00:16:39.5
20:23:46.13 -04:11:11.4
20:37:38.50 +00:00:54.3
20:43:36.06 -00:01:45.2
20:39:57.41 +00:21:22.6
20:37:19.38 +00:10:11.5
20:15:52.15 -02:15:14.8
20:15:29.40 -03:06:16.4
20:24:11.19 -04:12:05.7
20:15:54.83 -02:17:07.2
20:15:01.73 -03:07:21.6
20:23:56.65 -04:09:32.4
20:15:33.59 -02:06:17.0
20:15:46.96 -02:21:54.7
20:15:42.25 -02:50:35.1
20:37:37.61 +00:00:28.4
20:16:11.07 -02:44:06.9
20:15:57.81 -02:22:40.1
20:37:35.57 -00:01:18.0
20:38:07.64 +00:19:55.7
20:23:30.57 -04:14:23.9
20:38:48.40 +00:18:30.8
20:15:31.14 -02:21:26.8
20:15:06.12 -02:36:09.6
20:15:36.95 -02:13:04.3
20:13:58.83 -03:12:40.4
20:37:19.37 +00:00:11.1
20:16:03.62 -02:36:58.2
20:16:05.66 -02:28:02.1
20:16:05.93 -02:56:55.1
20:14:43.14 -02:36:01.6
20:14:21.22 -01:57:46.7
20:23:48.53 -04:14:03.1
20:23:39.55 -04:14:24.3
20:15:20.88 -02:48:06.9
20:15:44.99 -02:44:46.7
20:15:32.14 -02:58:22.3
20:15:54.39 -02:22:34.8
20:15:54.16 -02:12:26.6
20:15:22.65 -02:26:19.2
20:15:28.95 -02:25:48.0
20:16:03.80 -02:20:06.7
20:15:32.62 -02:56:38.8
20:15:24.24 -02:21:57.1
20:16:21.09 -02:54:29.5
20:15:51.41 -02:27:26.6
20:15:24.74 -02:50:50.2
20:14:16.12 -03:11:57.0
20:37:26.59 +00:07:23.6
20:15:28.25 -02:21:20.0
20:14:52.21 -03:10:30.0
20:15:04.32 -02:26:07.7
20:23:56.24 -04:17:37.3
20:14:34.94 -03:07:41.5
20:15:59.41 -02:20:20.6
20:15:48.69 -02:12:45.0
20:15:08.67 -02:05:03.4
20:14:17.31 -03:10:38.9
20:15:11.65 -02:14:55.3
20:15:30.95 -02:42:46.9
20:14:59.73 -03:05:25.5
20:15:23.51 -02:25:46.8
20:16:07.67 -02:50:01.0
20:15:40.01 -02:56:51.0
20:15:29.25 -03:03:15.6
20:15:43.53 -02:27:24.4
20:13:59.50 -01:57:29.9
20:14:13.24 -01:54:59.0
20:15:02.84 -02:33:54.1
20:15:09.85 -02:42:23.3
20:15:41.35 -02:23:51.8
20:15:03.28 -02:27:48.4
20:15:09.74 -02:23:39.6
20:14:28.84 -02:03:57.9
20:15:23.99 -03:00:21.0
20:13:48.46 -03:17:54.0
20:15:18.56 -02:37:14.3
20:15:47.35 -02:45:43.9
20:16:22.59 -02:35:44.5
20:15:49.44 -02:25:51.1
20:23:22.12 -04:12:03.1
20:15:08.97 -02:37:32.6
20:43:37.92 -00:01:47.3
20:16:18.20 -02:31:01.4
20:15:33.54 -02:19:06.4
20:15:42.22 -02:44:08.0
20:15:50.06 -02:13:26.2
20:38:10.42 +00:12:19.4
20:15:39.52 -02:31:07.2
20:16:31.34 -02:51:47.2
###################################################################################
20:36:36.83 +00:16:14.5 -- not an asteroid (will add it to exclusion list)
20:16:06.46 -02:56:32.1 -- not an asteroid (will add it to exclusion list)
20:16:20.76 -02:29:11.0 -- not an asteroid (will add it to exclusion list)
20:16:31.57 -02:48:05.6 -- not an asteroid (will add it to exclusion list)
20:36:48.45 +00:16:39.5 -- not an asteroid (will add it to exclusion list)
20:23:46.13 -04:11:11.4 -- not an asteroid (will add it to exclusion list)
20:37:38.50 +00:00:54.3 -- not an asteroid (will add it to exclusion list)
20:43:36.06 -00:01:45.2 -- not an asteroid (will add it to exclusion list)
20:39:57.41 +00:21:22.6 -- not an asteroid (will add it to exclusion list)
20:37:19.38 +00:10:11.5 -- not an asteroid (will add it to exclusion list)
20:15:52.15 -02:15:14.8 -- not an asteroid (will add it to exclusion list)
20:15:29.40 -03:06:16.4 -- not an asteroid (will add it to exclusion list)
20:24:11.19 -04:12:05.7 -- not an asteroid (will add it to exclusion list)
20:15:54.83 -02:17:07.2 -- not an asteroid (will add it to exclusion list)
20:15:01.73 -03:07:21.6 -- asteroid (will NOT add it to exclusion list)
20:23:56.65 -04:09:32.4 -- not an asteroid (will add it to exclusion list)
20:15:33.59 -02:06:17.0 -- not an asteroid (will add it to exclusion list)
20:15:46.96 -02:21:54.7 -- not an asteroid (will add it to exclusion list)
20:15:42.25 -02:50:35.1 -- not an asteroid (will add it to exclusion list)
20:37:37.61 +00:00:28.4 -- not an asteroid (will add it to exclusion list)
20:16:11.07 -02:44:06.9 -- not an asteroid (will add it to exclusion list)
20:15:57.81 -02:22:40.1 -- not an asteroid (will add it to exclusion list)
20:37:35.57 -00:01:18.0 -- not an asteroid (will add it to exclusion list)
20:38:07.64 +00:19:55.7 -- not an asteroid (will add it to exclusion list)
20:23:30.57 -04:14:23.9 -- not an asteroid (will add it to exclusion list)
20:38:48.40 +00:18:30.8 -- not an asteroid (will add it to exclusion list)
20:15:31.14 -02:21:26.8 -- not an asteroid (will add it to exclusion list)
20:15:06.12 -02:36:09.6 -- asteroid (will NOT add it to exclusion list)
20:15:36.95 -02:13:04.3 -- not an asteroid (will add it to exclusion list)
20:13:58.83 -03:12:40.4 -- asteroid (will NOT add it to exclusion list)
20:37:19.37 +00:00:11.1 -- not an asteroid (will add it to exclusion list)
20:16:03.62 -02:36:58.2 -- asteroid (will NOT add it to exclusion list)
20:16:05.66 -02:28:02.1 -- not an asteroid (will add it to exclusion list)
20:16:05.93 -02:56:55.1 -- not an asteroid (will add it to exclusion list)
20:14:43.14 -02:36:01.6 -- not an asteroid (will add it to exclusion list)
20:14:21.22 -01:57:46.7 -- not an asteroid (will add it to exclusion list)
20:23:48.53 -04:14:03.1 -- not an asteroid (will add it to exclusion list)
20:23:39.55 -04:14:24.3 -- not an asteroid (will add it to exclusion list)
20:15:20.88 -02:48:06.9 -- not an asteroid (will add it to exclusion list)
20:15:44.99 -02:44:46.7 -- asteroid (will NOT add it to exclusion list)
20:15:32.14 -02:58:22.3 -- not an asteroid (will add it to exclusion list)
20:15:54.39 -02:22:34.8 -- not an asteroid (will add it to exclusion list)
20:15:54.16 -02:12:26.6 -- not an asteroid (will add it to exclusion list)
20:15:22.65 -02:26:19.2 -- not an asteroid (will add it to exclusion list)
20:15:28.95 -02:25:48.0 -- not an asteroid (will add it to exclusion list)
20:16:03.80 -02:20:06.7 -- not an asteroid (will add it to exclusion list)
20:15:32.62 -02:56:38.8 -- not an asteroid (will add it to exclusion list)
20:15:24.24 -02:21:57.1 -- not an asteroid (will add it to exclusion list)
20:16:21.09 -02:54:29.5 -- not an asteroid (will add it to exclusion list)
20:15:51.41 -02:27:26.6 -- not an asteroid (will add it to exclusion list)
20:15:24.74 -02:50:50.2 -- not an asteroid (will add it to exclusion list)
20:14:16.12 -03:11:57.0 -- not an asteroid (will add it to exclusion list)
20:37:26.59 +00:07:23.6 -- not an asteroid (will add it to exclusion list)
20:15:28.25 -02:21:20.0 -- not an asteroid (will add it to exclusion list)
20:14:52.21 -03:10:30.0 -- asteroid (will NOT add it to exclusion list)
20:15:04.32 -02:26:07.7 -- not an asteroid (will add it to exclusion list)
20:23:56.24 -04:17:37.3 -- not an asteroid (will add it to exclusion list)
20:14:34.94 -03:07:41.5 -- not an asteroid (will add it to exclusion list)
20:15:59.41 -02:20:20.6 -- not an asteroid (will add it to exclusion list)
20:15:48.69 -02:12:45.0 -- not an asteroid (will add it to exclusion list)
20:15:08.67 -02:05:03.4 -- not an asteroid (will add it to exclusion list)
20:14:17.31 -03:10:38.9 -- not an asteroid (will add it to exclusion list)
20:15:11.65 -02:14:55.3 -- not an asteroid (will add it to exclusion list)
20:15:30.95 -02:42:46.9 -- asteroid (will NOT add it to exclusion list)
20:14:59.73 -03:05:25.5 -- not an asteroid (will add it to exclusion list)
20:15:23.51 -02:25:46.8 -- not an asteroid (will add it to exclusion list)
20:16:07.67 -02:50:01.0 -- not an asteroid (will add it to exclusion list)
20:15:40.01 -02:56:51.0 -- not an asteroid (will add it to exclusion list)
20:15:29.25 -03:03:15.6 -- not an asteroid (will add it to exclusion list)
20:15:43.53 -02:27:24.4 -- asteroid (will NOT add it to exclusion list)
20:13:59.50 -01:57:29.9 -- not an asteroid (will add it to exclusion list)
20:14:13.24 -01:54:59.0 -- not an asteroid (will add it to exclusion list)
20:15:02.84 -02:33:54.1 -- asteroid (will NOT add it to exclusion list)
20:15:09.85 -02:42:23.3 -- asteroid (will NOT add it to exclusion list)
20:15:41.35 -02:23:51.8 -- not an asteroid (will add it to exclusion list)
20:15:03.28 -02:27:48.4 -- not an asteroid (will add it to exclusion list)
20:15:09.74 -02:23:39.6 -- not an asteroid (will add it to exclusion list)
20:14:28.84 -02:03:57.9 -- not an asteroid (will add it to exclusion list)
20:15:23.99 -03:00:21.0 -- not an asteroid (will add it to exclusion list)
20:13:48.46 -03:17:54.0 -- asteroid (will NOT add it to exclusion list)
20:15:18.56 -02:37:14.3 -- asteroid (will NOT add it to exclusion list)
20:15:47.35 -02:45:43.9 -- not an asteroid (will add it to exclusion list)
20:16:22.59 -02:35:44.5 -- not an asteroid (will add it to exclusion list)
20:15:49.44 -02:25:51.1 -- not an asteroid (will add it to exclusion list)
20:23:22.12 -04:12:03.1 -- not an asteroid (will add it to exclusion list)
20:15:08.97 -02:37:32.6 -- asteroid (will NOT add it to exclusion list)
20:43:37.92 -00:01:47.3 -- not an asteroid (will add it to exclusion list)
20:16:18.20 -02:31:01.4 -- not an asteroid (will add it to exclusion list)
20:15:33.54 -02:19:06.4 -- not an asteroid (will add it to exclusion list)
20:15:42.22 -02:44:08.0 -- asteroid (will NOT add it to exclusion list)
20:15:50.06 -02:13:26.2 -- not an asteroid (will add it to exclusion list)
20:38:10.42 +00:12:19.4 -- not an asteroid (will add it to exclusion list)
20:15:39.52 -02:31:07.2 -- asteroid (will NOT add it to exclusion list)
20:16:31.34 -02:51:47.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:13:59.50 -01:57:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:13.24 -01:54:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:16.12 -03:11:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:17.31 -03:10:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:21.22 -01:57:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:28.84 -02:03:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:34.94 -03:07:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:43.14 -02:36:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:59.73 -03:05:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:03.28 -02:27:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:04.32 -02:26:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:08.67 -02:05:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:09.74 -02:23:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:11.65 -02:14:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:20.88 -02:48:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:22.65 -02:26:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:23.51 -02:25:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:23.99 -03:00:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:24.24 -02:21:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:24.74 -02:50:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:28.25 -02:21:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:28.95 -02:25:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:29.25 -03:03:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:29.40 -03:06:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:31.14 -02:21:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:32.14 -02:58:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:32.62 -02:56:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:33.54 -02:19:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:33.59 -02:06:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:36.95 -02:13:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:40.01 -02:56:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:41.35 -02:23:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:42.25 -02:50:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:46.96 -02:21:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:47.35 -02:45:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:48.69 -02:12:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:49.44 -02:25:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:50.06 -02:13:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:51.41 -02:27:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:52.15 -02:15:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:54.16 -02:12:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:54.39 -02:22:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:54.83 -02:17:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:57.81 -02:22:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:59.41 -02:20:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:03.80 -02:20:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:05.66 -02:28:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:05.93 -02:56:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:06.46 -02:56:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:07.67 -02:50:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:11.07 -02:44:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:18.20 -02:31:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:20.76 -02:29:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:21.09 -02:54:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:22.59 -02:35:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:31.34 -02:51:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:31.57 -02:48:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:22.12 -04:12:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:30.57 -04:14:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:39.55 -04:14:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:46.13 -04:11:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:48.53 -04:14:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:56.24 -04:17:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:56.65 -04:09:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:11.19 -04:12:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:36.83 +00:16:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:48.45 +00:16:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:19.37 +00:00:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:19.38 +00:10:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:26.59 +00:07:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:35.57 -00:01:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:37.61 +00:00:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:38.50 +00:00:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:07.64 +00:19:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:10.42 +00:12:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:48.40 +00:18:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:57.41 +00:21:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:36.06 -00:01:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:37.92 -00:01:47.3 -- 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)
20:13:59.50 -01:57:29.9 -- not a known variable star
20:14:13.24 -01:54:59.0 -- not a known variable star
20:14:16.12 -03:11:57.0 -- not a known variable star
20:14:17.31 -03:10:38.9 -- not a known variable star
20:14:21.22 -01:57:46.7 -- not a known variable star
20:14:28.84 -02:03:57.9 -- not a known variable star
20:14:34.94 -03:07:41.5 -- not a known variable star
20:14:43.14 -02:36:01.6 -- not a known variable star
20:14:59.73 -03:05:25.5 -- not a known variable star
20:15:03.28 -02:27:48.4 -- not a known variable star
20:15:04.32 -02:26:07.7 -- not a known variable star
20:15:08.67 -02:05:03.4 -- not a known variable star
20:15:09.74 -02:23:39.6 -- not a known variable star
20:15:11.65 -02:14:55.3 -- not a known variable star
20:15:20.88 -02:48:06.9 -- not a known variable star
20:15:22.65 -02:26:19.2 -- not a known variable star
20:15:23.51 -02:25:46.8 -- not a known variable star
20:15:23.99 -03:00:21.0 -- a known variable star
20:15:24.24 -02:21:57.1 -- not a known variable star
20:15:24.74 -02:50:50.2 -- not a known variable star
20:15:28.25 -02:21:20.0 -- not a known variable star
20:15:28.95 -02:25:48.0 -- not a known variable star
20:15:29.25 -03:03:15.6 -- not a known variable star
20:15:29.40 -03:06:16.4 -- not a known variable star
20:15:31.14 -02:21:26.8 -- not a known variable star
20:15:32.14 -02:58:22.3 -- a known variable star
20:15:32.62 -02:56:38.8 -- not a known variable star
20:15:33.54 -02:19:06.4 -- not a known variable star
20:15:33.59 -02:06:17.0 -- not a known variable star
20:15:36.95 -02:13:04.3 -- not a known variable star
20:15:40.01 -02:56:51.0 -- not a known variable star
20:15:41.35 -02:23:51.8 -- not a known variable star
20:15:42.25 -02:50:35.1 -- not a known variable star
20:15:46.96 -02:21:54.7 -- not a known variable star
20:15:47.35 -02:45:43.9 -- not a known variable star
20:15:48.69 -02:12:45.0 -- not a known variable star
20:15:49.44 -02:25:51.1 -- not a known variable star
20:15:50.06 -02:13:26.2 -- not a known variable star
20:15:51.41 -02:27:26.6 -- not a known variable star
20:15:52.15 -02:15:14.8 -- not a known variable star
20:15:54.16 -02:12:26.6 -- not a known variable star
20:15:54.39 -02:22:34.8 -- not a known variable star
20:15:54.83 -02:17:07.2 -- not a known variable star
20:15:57.81 -02:22:40.1 -- not a known variable star
20:15:59.41 -02:20:20.6 -- not a known variable star
20:16:03.80 -02:20:06.7 -- not a known variable star
20:16:05.66 -02:28:02.1 -- not a known variable star
20:16:05.93 -02:56:55.1 -- not a known variable star
20:16:06.46 -02:56:32.1 -- not a known variable star
20:16:07.67 -02:50:01.0 -- not a known variable star
20:16:11.07 -02:44:06.9 -- not a known variable star
20:16:18.20 -02:31:01.4 -- not a known variable star
20:16:20.76 -02:29:11.0 -- not a known variable star
20:16:21.09 -02:54:29.5 -- not a known variable star
20:16:22.59 -02:35:44.5 -- not a known variable star
20:16:31.34 -02:51:47.2 -- not a known variable star
20:16:31.57 -02:48:05.6 -- not a known variable star
20:23:22.12 -04:12:03.1 -- a known variable star
20:23:30.57 -04:14:23.9 -- not a known variable star
20:23:39.55 -04:14:24.3 -- not a known variable star
20:23:46.13 -04:11:11.4 -- not a known variable star
20:23:48.53 -04:14:03.1 -- not a known variable star
20:23:56.24 -04:17:37.3 -- not a known variable star
20:23:56.65 -04:09:32.4 -- not a known variable star
20:24:11.19 -04:12:05.7 -- a known variable star
20:36:36.83 +00:16:14.5 -- not a known variable star
20:36:48.45 +00:16:39.5 -- not a known variable star
20:37:19.37 +00:00:11.1 -- not a known variable star
20:37:19.38 +00:10:11.5 -- not a known variable star
20:37:26.59 +00:07:23.6 -- not a known variable star
20:37:35.57 -00:01:18.0 -- not a known variable star
20:37:37.61 +00:00:28.4 -- not a known variable star
20:37:38.50 +00:00:54.3 -- not a known variable star
20:38:07.64 +00:19:55.7 -- not a known variable star
20:38:10.42 +00:12:19.4 -- not a known variable star
20:38:48.40 +00:18:30.8 -- not a known variable star
20:39:57.41 +00:21:22.6 -- not a known variable star
20:43:36.06 -00:01:45.2 -- not a known variable star
20:43:37.92 -00:01:47.3 -- not a known variable star
Found 75 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
79 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 79 (excluding asteroids and hot pixels, 75 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)2461239.76693241 -observatory V36
07:12:34.15 +17:30:56.6 Mercury (4.0mag)
10:44:04.30 +09:05:40.0 Venus (-4.2mag)
04:47:38.22 +22:18:18.7 Mars (1.3mag)
08:23:53.18 +19:48:12.4 Jupiter (-1.8mag)
00:56:31.59 +03:22:19.7 Saturn (0.7mag)
04:08:40.89 +20:48:56.4 Uranus (5.8mag)
00:16:55.65 +00:19:36.3 Neptune (7.7mag)
20:30:10.36 -23:21:29.3 Pluto (14.4mag)
11:07:16.66 +03:07:59.9 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jul 18 06:58 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461239.76693241:
08:23:50.09 +19:48:24.1 Io (6.0mag)
08:24:04.56 +19:47:28.7 Europa (6.3mag)
08:24:09.44 +19:47:08.3 Ganymede (5.6mag)
08:23:27.12 +19:49:53.4 Callisto (6.8mag)
08:22:03.99 +19:35:55.4 Himalia (15.7mag)
08:23:52.26 +19:48:17.0 Thebe (16.6mag)
08:21:25.01 +19:38:39.4 Elara (17.7mag)
08:27:38.98 +19:38:10.0 Pasiphae (17.9mag)
08:28:23.38 +19:54:29.4 Carme (19.0mag)
00:56:41.86 +03:22:27.1 Titan (8.5mag)
00:56:31.30 +03:22:29.9 Rhea (9.8mag)
00:55:57.08 +03:20:10.2 Iapetus (11.2mag)
00:56:18.45 +03:22:10.8 Hyperion (14.5mag)
00:56:21.72 +03:18:24.6 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 06:58 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.76693241:
17:58:53.26 -31:05:19.2 JWST
16:13:05.34 +49:48:04.5 Chandra
22:29:20.81 +57:15:23.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 06:58 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.76693241 -observatory V36
02:47:19.39 +15:20:23.2 17.8mag P/1996 R2 (Lagerkvist)
18:12:09.44 -34:32:35.6 13.8mag P/2010 H2 (Vales)
06:33:34.10 -68:17:06.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:30.40 +32:35:05.3 17.6mag C/2017 K2 (PANSTARRS)
02:28:09.55 +21:14:59.5 15.8mag P/2021 N1 (ZTF)
22:54:30.97 +32:13:29.6 17.3mag C/2022 E2 (ATLAS)
06:21:19.93 +26:50:49.1 16.7mag C/2022 N2 (PANSTARRS)
10:02:28.86 +29:25:27.0 16.9mag C/2022 QE78 (ATLAS)
09:14:53.27 +05:07:59.1 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.74 -11:35:06.1 17.8mag P/2023 B1 (PANSTARRS)
21:39:16.68 +67:29:04.1 17.9mag C/2023 H5 (Lemmon)
16:16:11.74 -10:53:47.2 14.0mag C/2023 R1 (PANSTARRS)
08:14:36.96 +66:08:56.7 17.9mag C/2024 A1 (ATLAS)
07:43:01.92 +30:23:39.8 14.8mag C/2024 E1 (Wierzchos)
15:12:48.33 +15:30:01.8 17.6mag C/2024 G6 (ATLAS)
19:30:59.86 +40:48:53.2 13.7mag C/2024 J3 (ATLAS)
21:38:53.33 +47:07:55.7 17.8mag C/2024 R4 (PANSTARRS)
04:57:01.33 -13:28:08.5 15.7mag C/2024 T5 (ATLAS)
06:41:00.55 +27:44:48.2 18.0mag C/2025 J1 (Borisov)
07:19:39.43 -13:38:05.3 16.9mag C/2025 R3 (PANSTARRS)
10:05:29.68 +22:04:40.7 17.5mag C/2025 V2 (Rankin)
12:47:31.55 +03:34:29.3 17.0mag C/2025 Y1 (ATLAS)
16:31:03.68 +79:07:45.9 17.2mag C/2026 A2 (Bok)
02:54:06.54 +45:33:55.0 16.8mag C/2026 B2 (Sun-Gao)
11:30:45.96 +05:51:53.7 17.0mag A/2026 E1
21:31:08.81 -18:06:54.6 7.1mag 10P/Tempel
11:17:18.43 -02:14:40.4 16.2mag 29P/Schwassmann-Wachmann
04:11:27.25 +30:23:51.4 17.9mag 47P/Ashbrook-Jackson
10:24:34.41 +11:28:26.7 17.1mag 63P/Wild
00:51:23.50 -05:02:47.8 15.5mag 65P/Gunn
04:46:28.52 +20:31:34.8 13.7mag 78P/Gehrels
02:34:40.11 +11:38:41.0 16.4mag 88P/Howell
06:58:47.35 +29:59:00.4 15.8mag 93P/Lovas
04:46:53.42 +31:19:48.8 16.7mag 114P/Wiseman-Skiff
08:28:01.43 +29:46:00.6 15.2mag 123P/West-Hartley
11:03:00.01 -02:01:05.7 16.9mag 124P/Mrkos
05:04:22.63 +21:00:37.0 16.2mag 128P/Shoemaker-Holt
05:51:04.67 +19:36:47.9 17.8mag 131P/Mueller
07:41:43.42 +15:15:30.7 16.5mag 141P-D/Machholz
03:20:18.04 -20:45:04.0 15.1mag 161P/Hartley-IRAS
06:01:37.78 +35:29:46.3 15.5mag 162P/SidingSpring
18:39:19.45 +20:30:36.6 14.0mag 169P/NEAT
01:59:34.37 +08:24:26.6 17.6mag 220P/McNaught
16:35:32.56 -08:44:37.1 17.2mag 235P/LINEAR
09:01:50.25 +32:32:31.1 18.0mag 240P/NEAT
20:37:57.17 -51:08:36.4 17.8mag 259P/Garradd
02:21:36.67 +15:47:26.2 15.6mag 260P/McNaught
06:01:20.91 +37:23:09.8 17.3mag 295P/LINEAR
15:06:33.44 +05:19:30.7 17.6mag 391P/Kowalski
08:41:44.94 +19:20:47.3 17.9mag 450P/LONEOS
08:04:07.50 +38:33:08.5 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 06:58 comets.txt
############################################################
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 06:58 asassn_transients_list.txt
############################################################
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 06:58 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:40:11.159 -09:00:57.92 AT 2026swa 2026-06-27.33 23.1049
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
-rw-r--r-- 1 apache apache 89K Jul 18 06:58 tns_transients_list.txt
