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M

M. Gromadzki

university of warsaw
H指数:37
被引数:5,896

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SN 2023taz: Implications for the UV Diversity of Superluminous Supernovae

SN 2023taz:对超亮超新星紫外多样性的启示

2026-04-150
OA
AT 2024wpp: An Extremely Luminous Fast Ultraviolet Transient Powered by Accretion onto a Black Hole

AT 2024wpp:一个由物质吸积到黑洞上驱动的极端明亮快速紫外暂现体

2026-04-100
OA
Mass Production of 2023 KMTNet Microlensing Planets. I. Low Mass Ratio

2023年KMTNet微引力透镜行星的大规模生产。I. 低质量比

2026-04-010
OAAI
SN 2021aaev: A Hydrogen-rich Superluminous Supernova with Early Flash and Long-lived Circumstellar Interaction in an Unusual Host Environment

SN 2021aaev:一颗具有早期闪光和长期 circumstellar interaction 的氢富超亮超新星,其宿主环境特殊

2026-03-020
OAAI
SN 2024abvb: a Type Ibn/Icn supernova with evidence of helium and an extreme offset from its host galaxy

SN 2024abvb:一颗具有氦元素证据且偏离宿主星系极远的Ibn/Icn型超新星

2026-02-260
OA
A free-floating-planet microlensing event caused by a Saturn-mass object

由土星质量物体引起的自由漂浮行星微透镜事件

Science
IF45.8
2026-01-010
PRE
SN 2020bij and a Possible Slow-rise High-velocity Subclass of Type IIP Supernovae

SN 2020bij及IIP型超新星可能的缓慢上升高速度亚类

2026-01-010
OAAI
KMT-2022-BLG-1818Lb; c: A Cold Super-Jupiter with a Saturn Sibling

KMT-2022-BLG-1818Lb; c: 一颗冷态超木星,其拥有一个土星级的兄弟姐妹

2025-12-170
OAAI
Detection of disk-jet coprecession in a tidal disruption event

潮汐瓦解事件中盘-喷流共进动的探测

2025-12-100
PRE
GRB 241105A: a test case for GRB classification and rapid r-process nucleosynthesis channels

GRB 241105A:GRB分类和快速<i>r</i>-过程核合成通道的一个测试案例

2025-11-010
PRE
SN 2024bfu, SN 2025qe, and the early light curves of type Iax supernovae

SN 2024bfu、SN 2025qe以及Iax型超新星早期光曲线

2025-11-011
OAAI
Microlensing Optical Depth; Event Rate; and Limits on Compact Objects in Dark Matter Based on 20 Yr of OGLE Observations of the Small Magellanic Cloud

微透镜光学深度;事件率;以及基于20年OGLE对小麦哲伦星云的观测对暗物质中致密物体的限制

2025-09-150
OAAI
The case of AT2022wtn: a tidal disruption event in an interacting galaxy

AT2022wtn案例:一个发生在相互作用星系中的潮汐瓦解事件

2025-05-080
OA
Asteroseismology of Long-period Variables with OGLE-IV Data: Using Global Seismic Parameters as Luminosity Indicators

长周期变星的星震学研究:使用OGLE-IV数据,将全局星震参数作为光度指示器

2025-04-280
OA
Gaia20bdk-New FU Ori-type star in the Sh 2-301 star-forming region
2025-03-120
OA
The diversity of strongly interacting Type IIn supernovae
2025-02-270
PRE
Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc

超亮超新星爆发前一年内的喷发质量损失:I. SN 2020xga和SN 2022xgc案例

2025-02-240
OA
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases
2025-02-190
OA
ZTF SN Ia DR2: Searching for late-time interaction signatures in Type Ia supernovae from the Zwicky Transient Facility
2025-02-141
OA