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 300017020 M87_SW_ARM 187.66044 12.35797 187.02767 12.63407 182.03129 14.36832 283.65656 74.44621 120.27824 60653.09866 2024-12-09 02:22:04 60655.10838 2024-12-11 02:36:04 82.049 72.000 82.049 79.890 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 79.890 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-12-21 09:12:59 2025-12-27 00:00:00 2024-12-22 09:12:59 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000035 We propose a mosaic of XRISM/Resolve pointings designed to study supermassive black hole feedback in the nearest and second brightest cool core cluster in spatially resolved detail. The most striking features in M87 are the 6 arcmin-long, X-ray bright arms thought to be filaments of multi-phase, metal-rich gas uplifted by the buoyant AGN radio lobes. XRISM measurements will reveal the kinematics of this uplift and quantify the amount of metals being transported outwards by the AGN. The relatively low ambient temperature of M87 corresponds to a line-rich spectrum that will perfectly showcase the soft X-ray capabilities of Resolve. GROUPS AND CLUSTERS OF GALAXIES 3 A XRISM Collaboration JAP 0 NOR SUPERMASSIVE BLACK HOLE FEEDBACK IN M87 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300017020/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300017020'

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