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 202002010 NGC6240 253.24585 2.40165 252.61645 2.48336 251.50634 24.77171 20.73 27.29087 110.23724 61070.11880 2026-01-30 02:51:04 61075.00977 2026-02-04 00:14:04 229.187 225.000 229.187 226.476 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 226.525 0.046 0.000 0.000 11110 313430 11310 PROCESSED 2026-02-11 09:54:10 2099-12-31 00:00:00 2026-02-12 09:54:11 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022048 We propose Resolve measurements of Fe K lines in to determine whether the starburst wind in NGC 6240 can drive a quenching outflow. NGC 6240 is the archetypal major merger, with a starburst, two AGN, and a molecular outflow of around 4000 solar masses per year coincident with the starburst that will rapidly quench the galaxy. If the starburst cannot drive the wind, then the AGN must. These data will also enable the kinematic separation of the dual AGN in Fe Ka, making NGC 6240 (where these nuclei are resolved by Chandra) a Rosetta stone for interpreting kinematic signatures of candidate dual or binary AGN in more distant systems. Finally, high-resolution spectra from the starburst wind will also constrain the metal outflow rate, key to measuring the cumulative enrichment of the cosmic web. NON-JET-DOMINATED AGN 2 B EDMUND HODGES-KLUCK USA 2 NOR DOES A STARBURST DRIVE THE GALACTIC WIND IN NGC 6240? processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202002010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202002010'

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