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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