Showing results 1 to 11 out of 11
AT 2024nqr / ZTF24aauekqv and AT 2024pgd / ZTF24aauywft, two ongoing transients towards a z = 0.089 galaxy
Source Group: ZTF
Related Objects:
2024nqr [ZTF24aauekqv]
, RA, DEC:15:12:27.278, +32:32:44.54
(228.113659, 32.545705)
Redshift:
Type:
2024pgd [ZTF24aauywft]
RA, DEC:15:12:26.332, +32:32:44.29
(228.109717, 32.545636)
Redshift:
Type:
We report on two ongoing transient events separated by ~12 arcsec, towards Seyfert 2 galaxy 2MASX J15122674+3232460, the brightest member of a group at z = 0.089. Follow-up observations of these tran…
Discovery of A Highly Magnified Transient at Redshift z = 3.78 in GLASS JWST NIRISS Imaging
Related Objects:
We report the discovery of a highly magnified transient (AT 2023mlz) in an arc at redshift z=3.784 in GLASS (PI: Treu) NIRISS observations of the Abell 2744 galaxy-cluster field taken on 2023 July 7.
SN H0pe: three images of a SN detected near the central region of the galaxy cluster field PLCK G165.7+67.0
Related Objects:
PLCK G165.7+67.0 [G165 b]
RA, DEC:00:00:00.000,
(0.000000, 0.000000)
Redshift:
Type:
PLCK G165.7+67.0 [G165 b]
We discovered a new transient in James Webb Space Telescope NIRCam imaging in the field of a massive galaxy cluster.
A Transient in JWST DD NIRCam Imaging of Abell 2744 Galaxy-Cluster Field
Related Objects:
Related Notes:
We report the detection of a new transient in NIRCam imaging of the Abell 2744 galaxy-cluster field taken on December 6, 2022 (UT) by the JWST DDT program 2756 (PI: Wenlei Chen). The transient was de…
Transient Candidates in JWST DD NIRCam Imaging of Abell 2744 Galaxy-Cluster Field
We report on the detection of two new transients in NIRCam imaging of the Abell 2744 galaxy-cluster field taken on October 20, 2022 (UT) by JWST DDT program 2756 (PI: Wenlei Chen). A first transient …
Multiple Images of SN 2022qmx (“SN Zwicky”) Resolved in HST Observations
Related Objects:
Related Notes:
The 4 images of gravitationally lensed SNIa 2022qmx (aka “SN Zwicky”; Goobar et al. AstroNote 2022-180) are resolved in HST observations from GO program 16264 (PI: Pierel). The data include F475W, F6…
Keck NIRC2+LGS Imaging Observations of SN 2022qmx (“SN Zwicky”)
Source Group: ZTF
Related Objects:
2022qmx [ZTF22aaylnhq]
RA, DEC:17:35:44.328, +04:49:56.86
(263.934702, 4.832460)
Redshift:0.35
Type:SN Ia
Related Notes:
Keck II observations in J and Ks bands of the strongly lensed Type Ia SN 2020qmx ("SN Zwicky"; Goobar et al. AstroNote 2022-180) show that SN Zwicky is multiply lensed with 4 images of the supernova …
Likely Supernova at z > 1 in the MACS J0257.1-2325 Galaxy-Cluster Field
Related Objects:
SN Zwicky (SN2022qmx): a Strongly Lensed Type Ia at z=0.35 discovered by ZTF
Source Group: ZTF
Related Objects:
2022qmx [ZTF22aaylnhq]
RA, DEC:17:35:44.328, +04:49:56.86
(263.934702, 4.832460)
Redshift:0.35
Type:SN Ia
We report the first Zwicky Transient Facility detection of a strongly gravitationally lensed Type Ia supernova.
Strongly Lensed SN in MACS 2129 Galaxy-Cluster Field
Related Objects:
Observations of lensed supernova candidate AT 2021vkz (ZTF21abqoivk) with the Liverpool Telescope
Related Objects:
2021vkz [ZTF21abqoivk]
RA, DEC:23:03:27.102, +07:56:33.55
(345.862924, 7.942652)
Redshift:0.15
Type:SN Ia
Imaging observations of strong gravitationally-lensed supernova candidate AT 2021vkz (ZTF21abqoivk) with the Liverpool Telescope.
Most Viewed
Discovery of Possible Transient in JWST NIRCam Images of SDSS J141930.11+525159.3
Early multiband light curve of SN 2023ixf
LT Classification of SN 2023ixf as a Type II Supernova in M101
Classification of SN 2020jfo (ZTF20aaynrrh) as a young Type II supernova
SN 2023tyk: discovery to spectroscopic classification performed fully automatically
ATLAS20ktt (AT2020hvp): discovery of a candidate supernova in NGC 6118 (27 Mpc)
Onset of SN 2023ixf observed over East Asian longitudes
ePESSTO+ re-classification of AT2019xis as a light echo of SN 1987A in the LMC.
ATLAS20qoq (AT2020nlb): discovery of a candidate SN in MESSIER 85 (17 Mpc)
Fast Radio Bursts (FRBs) now reported to and distributed via the TNS