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 201073010 SERPENS_X-1 279.99033 5.03594 279.37364 4.9891 281.29588 28.08433 36.11839 4.8417 257.94823 60600.90074 2024-10-17 21:37:04 60604.98060 2024-10-21 23:32:04 172.513 150.000 172.513 19.212 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31300010 320000A0 153.375 0.000 0.000 19.212 11110 313430 11310 PROCESSED 2024-10-26 11:43:52 2025-10-31 00:00:00 2024-10-27 11:43:53 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000012057 Serpens X-1 is a persistently accreting neutron star (NS) with the first confirmed relativistically broadened Fe line for such systems. However, there remains conflicting reports of key parameters, such as the position of the inner accretion disk and inclination. These quantities can be determined from resolving the red- and blue-wings of the Fe line profile, which are most sensitive to the gravitational redshift and Doppler effects, respectively. Further, the Fe line has a unique double-peaked profile which can be due to high disk density effects causing the Fe XXV and XXVI lines to be produced at a similar strength. We request a 300 ks observation of the source to reveal the Doppler and relativistic effects that shape the line profile and further our understanding of the accretion flow. BH AND NS BINARIES 2 A RENEE LUDLAM USA 1 NOR RESOLVING RELATIVISTIC EFFECTS IN THE ACCRETION DISK OF SERPENS X-1 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201073010/ WINDOW2BURST WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201073010'

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