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 203153010 X_PERSEI 58.84409 31.04557 58.0611 30.89993 63.20834 10.45836 163.08017 -17.13758 73.32797 61303.80838 2026-09-20 19:24:04 61304.09796 2026-09-21 02:21:04 11.247 10.000 11.247 9.023 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 9.651 9.023 0.000 0.000 11110 313430 11310 PROCESSED 2026-10-01 06:57:15 2027-10-07 00:00:00 2026-10-02 06:57:16 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000034042 Clumping is known to occur in the circumstellar environments of massive binaries and may also be present in Be discs. In this context, fluorescent Fe~K$\alpha$ emission can provide a sensitive probe of cold, dense structures embedded in a more tenuous medium. X Persei spectra are typically poor in emission lines, and to our knowledge no persistent narrow Fe~K$\alpha$ line has been reported. However, NS spin phase-resolved spectroscopy of \xmmnewton and \chandra\ data revealed transient Fe~K$\alpha$ signatures that are otherwise diluted in phase-averaged spectra. Over the same spin cycle, the continuum components vary consistently with emission from an accretion-powered hotspot on the NS surface, whereas the origin of the soft excess remains unclear. These studies are currently limited by BH AND NS BINARIES 2 A GRACIELA SANJURJO EUR 3 NOR TRACING THE BE-STAR DECRETION DISC ENVIRONMENT AND NS SPIN VARIABILITY IN X PER WITHXRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203153010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203153010'

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