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
|
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| 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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