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 201036010 CIR_X-1 230.1686 -57.16715 229.19997 -56.98696 244.13233 -37.25036 322.11754 0.03783 103.57368 60719.27157 2025-02-13 06:31:04 60721.16741 2025-02-15 04:01:04 76.429 60.000 76.429 8.461 PX_NORMAL N Y Y N Y Y Y OFF OFF OFF OFF 2 31300010 320000A0 67.548 0.000 0.000 8.461 11110 313430 11310 PROCESSED 2025-02-19 12:37:56 2026-02-20 00:00:00 2025-02-20 12:37:57 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011196 In X-ray binaries, the presence of the excretion (outward) flow is theoretically envisioned as inevitable. The excretion flow has been entirely ignored despite its firm theoretical ground, but recent observations point toward the presence of it. Convincing evidence was obtained with the NICER observations of the neutron star binary Cir X-1. Physical properties of the excretion flow can be constrained with two high-resolution X-ray spectra taken at different orbital phases. The diagnostic requires a spectral resolution of R = E/DE ~ 10^3 in 2-8 keV band, which can only be achieved with Resolve. One of the two observations was already executed in the PV phase, and we propose the other one in the AO1 cycle, to verify the presence of the excretion flow. BH AND NS BINARIES 2 A NAGI ATSUCHI JAP 1 NOR ESTABLISHING THE PRESENCE OF EXCRETION FLOW IN X-RAY BINARIES WITH RESOLVE SPECTROSCOPY OF CIRCINUS X-1 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201036010/ WINDOW2BURST WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201036010'

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