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 202001010 NGC4839 194.30011 27.48879 193.69467 27.75888 181.16159 30.70684 48.99175 88.67014 133.82507 61010.67435 2025-12-01 16:11:04 61013.80838 2025-12-04 19:24:04 137.095 190.000 137.095 127.540 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 127.540 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-12-09 11:10:57 2099-12-31 00:00:00 2025-12-10 11:10:57 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022046 We propose to observe the inner part of the ram pressure stripped tail of the galaxy group NGC 4839, which is infalling into the Coma cluster, for 190ks with Resolve. A surface brightness fluctuation analysis of the inner tail with Chandra has revealed a turbulent Mach number of 0.5, which should result in a velocity dispersion of 320km/s. The low redshift of the system makes this the brightest stripped tail in X-rays and mitigates the complicating factor of XRISM's large PSF, which combined with its high metallicity of 0.8 Z_solar makes it the only tail whose velocity dispersion can be measured with a realistic exposure time with XRISM. This system therefore provides a unique opportunity to probe the generation of turbulence due to merging activity in galaxy clusters. GROUPS AND CLUSTERS OF GALAXIES 2 A STEPHEN WALKER USA 2 NOR XRISM OBSERVATIONS OF TURBULENCE IN A RAM PRESSURE STRIPPED GALAXY GROUP TAIL FALLING THROUGH THE COMA CLUSTER preprocessed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202001010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202001010'

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