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 300008010 T_CORONA_BOREALIS 239.87456 25.92151 239.35091 26.0623 230.09823 45.27585 42.37544 48.16595 321.17066 60488.00282 2024-06-27 00:04:04 60494.49171 2024-07-03 11:48:04 294.093 150.000 294.093 230.377 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 230.377 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-22 10:43:37 2025-08-31 00:00:00 2024-07-11 19:38:13 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000020 We propose to measure the gravitational redshift at the surface of a massive accreting white dwarf (WD) in T CrB. It is a hard X-ray luminous symbiotic recurrent nova, with an estimated WD mass of >1.15 Msun, above the likely upper limit of WD birth mass. If confirmed, it implies that the WD in T CrB is growing in mass, establishing a subset of symbiotic stars as a viable progenitor channel of Type Ia supernovae. The primary X-ray source is located just above the WD surface, and it is the latter that produces the reflection continuum and the Fe Kalpha and Kbeta fluorescent lines. Measuring the centroids of both will enable us to determine the ionization state of the WD photosphere and the WD mass. ACCRETING WHITE DWARFS AND NOVAE 3 A XRISM Collaboration JAP 0 NOR-TOO GRAVITATIONALLY REDSHIFTED 6.4 KEV LINE IN T CORONAE BOREALIS archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300008010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300008010'

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