DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
observation_id
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
exposure
awarded_exposure
resolve_exposure
xtend_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
xtend_number_modes
xtend_dataclass_file1
xtend_dataclass_file2
xtend_window1_exposure
xtend_window2_exposure
xtend_window1_burst_exposure
xtend_window2_burst_exposure
xtend_code
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
xtend_data_mode1
xtend_data_mode2
processing_count
remarks
1 203148010 HOLMBERG_IX_X-1 149.47125 69.06362 148.45321 69.3021 119.77204 51.69348 141.93341 41.07065 164.98533 61286.28130 2026-09-03 06:45:04 61288.26116 2026-09-05 06:16:04 127.316 90.000 127.316 112.338 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 112.338 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-09-18 23:24:03 2099-12-31 00:00:00 2026-09-19 23:24:04 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000032263 We propose a 90 ks XRISM observation of Holmberg IX X-1, a benchmark ultraluminous X-ray (ULX) source whose mechanical feedback, traced by a large ionized and optical and radio bubble, has yet to be directly linked to an active outflow. The source accretes persistently in the super-Eddington regime and is embedded in a bubble requiring substantial energy injection into the surrounding interstellar medium. However, the nature of the engine driving this feedback remains uncertain. A 90 ks Resolve exposure will either detect fast, highly ionized winds or place decisive limits on their kinetic power, allowing us to test whether present-day outflows can account for the observed bubble energetics and establish how ULXs impact their host galaxies. BH AND NS BINARIES 2 A PRIYANKA CHAKRABORTY USA 3 NOR CLOSING THE FEEDBACK GAP IN HOLMBERG IX X-1 WITH XRISM preprocessed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203148010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203148010'

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