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 | 201090010 | RT_CRU | 188.7239 | -64.56576 | 187.99863 | -64.29023 | 224.62522 | -53.38367 | 301.15622 | -1.75106 | 261.57714 | 60835.50005 | 2025-06-09 12:00:04 | 60839.83824 | 2025-06-13 20:07:04 | 177.706 | 150.000 | 177.706 | 153.453 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 153.453 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2025-07-14 13:53:03 | 2026-06-19 00:00:00 | 2025-06-18 14:16:23 | 03.02.014.010 | gen20241115_xtd20241115_rsl20241115 | Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 | 000012128 | The goal of the proposed XRISM observation is to show that high-resolution X-ray spectroscopy can directly reveal the mass of an accreting white dwarf (WD). By measuring the centroids of Fe Ka and Kb; fluorescent lines reflected from the WD, we will determine the gravitational redshift at the WD surface and hence the WD mass in RT Cru, the most hard-X-ray luminous symbiotic binary star. The mass of this WD is thought to be above the likely upper limit for its birth mass. Confirmation of this situation would imply that the mass is almost certainly increasing, establishing a subset of symbiotic stars as viable progenitors for some Type Ia supernovae. Because this project uses emission lines in the 6-7 keV range, it is minimally impacted by the Gate Valve remaining in the closed configuration | ACCRETING WHITE DWARFS AND NOVAE | 2 | A | JENNIFER SOKOLOSKI | USA | 1 | NOR | DIRECT MEASUREMENT OF WHITE DWARF MASSES WITH XRISM: GRAVITATIONALLY REDSHIFTED 6.4 KEV LINE IN RT CRU | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201090010/ | WINDOW1 | 2 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '201090010'
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